List of Solar System objects by size: Difference between revisions

From Wikipedia, the free encyclopedia
[pending revision][pending revision]
Content deleted Content added
Per the Non-free content criteria #10c, all non-free files on this page must have a specific non-free use rationale.
Line 78: Line 78:
| [[Star]]
| [[Star]]
|regular
|regular
|-style="background:#ddd;"
|-style="background:#ddd;"
|[[Jupiter]]
|[[Jupiter]]
|bgcolor=black|[[File:Jupiter by Cassini-Huygens.jpg|50px]]
|bgcolor=black|[[File:Jupiter by Cassini-Huygens.jpg|50px]]
Line 314: Line 314:
|[[Pluto]]<sup>R</sup><br><small> 134340</small>
|[[Pluto]]<sup>R</sup><br><small> 134340</small>
|bgcolor=black|[[File:Pluto-map-hs-2010-06-c180.jpg|50px]] <!-- HST / NASA -->
|bgcolor=black|[[File:Pluto-map-hs-2010-06-c180.jpg|50px]] <!-- HST / NASA -->
|1,161<ref name=young07>{{cite journal|bibcode=2007DPS....39.6205Y |title=Pluto's Radius|author=Young, Eliot F.; Young, L. A.; Buie, M. |journal=American Astronomical Society, DPS meeting #39, #62.05; Bulletin of the American Astronomical Society|volume=39|page=541|year=2007}}</ref></br>(w/o gas)
|1,161<ref name=young07>{{cite journal|bibcode=2007DPS....39.6205Y |title=Pluto's Radius|author=Young, Eliot F.; Young, L. A.; Buie, M. |journal=American Astronomical Society, DPS meeting #39, #62.05; Bulletin of the American Astronomical Society|volume=39|page=541|year=2007}}</ref><br />(w/o gas)
|0.181
|0.181
|7.15
|7.15
Line 420: Line 420:
|600–800<ref name=Sedna-LKBO>
|600–800<ref name=Sedna-LKBO>
{{cite book
{{cite book
| chapter = The largest Kuiper belt objects
| chapter = The largest Kuiper belt objects
| title = The Solar System Beyond Neptune
| title = The Solar System Beyond Neptune
| pages = 335–345
| pages = 335–345
| editor = M. Antonietta Barucci, Hermann Boehnhardt, Dale P. Cruikshank
| editor = M. Antonietta Barucci, Hermann Boehnhardt, Dale P. Cruikshank
| author = Michael E. Brown
| author = Michael E. Brown
| publisher = University of Arizona Press
| publisher = University of Arizona Press
| isbn = 0-8165-2755-5
| isbn = 0-8165-2755-5
| url = http://www.gps.caltech.edu/~mbrown/papers/ps/kbochap.pdf
| url = http://www.gps.caltech.edu/~mbrown/papers/ps/kbochap.pdf
| format = pdf
| format = pdf
}}
}}
</ref>
</ref>
Line 445: Line 445:
|bgcolor=black|[[File:1880-CT MBrown SPOTLIGHT medium.jpg|30px]]
|bgcolor=black|[[File:1880-CT MBrown SPOTLIGHT medium.jpg|30px]]
|≈600<ref name="Brown2011">{{cite web
|≈600<ref name="Brown2011">{{cite web
|year=2011
|year=2011
|title=The Surface Composition of Large Kuiper Belt Object 2007 OR10
|title=The Surface Composition of Large Kuiper Belt Object 2007 OR10
|publisher=Mike Brown's Website
|publisher=Mike Brown's Website
|author=[[Michael E. Brown]]; Burgasser, A.J.; Fraser W.C.
|author=[[Michael E. Brown]]; Burgasser, A.J.; Fraser W.C.
|url=http://www.gps.caltech.edu/~mbrown/papers/ps/or10.pdf
|url=http://www.gps.caltech.edu/~mbrown/papers/ps/or10.pdf
|arxiv=1108.1418
|arxiv=1108.1418
|accessdate=2011-08-08}}</ref>–710<ref name=Brown>Mike Brown, ''How many dwarf planets are there in the outer solar system?''[http://www.gps.caltech.edu/~mbrown/dps.html]</ref>
|accessdate=2011-08-08}}</ref>–710<ref name=Brown>Mike Brown, ''How many dwarf planets are there in the outer solar system?''[http://www.gps.caltech.edu/~mbrown/dps.html]</ref>
|0.094
|0.094
|0.904
|0.904
Line 478: Line 478:
|-style="background:#CCFFCC;"
|-style="background:#CCFFCC;"
|[[Ariel (moon)|Ariel]] <sup>‡</sup> <br><small> Uranus I</small>
|[[Ariel (moon)|Ariel]] <sup>‡</sup> <br><small> Uranus I</small>
|bgcolor=black|[[File:Ariel-NASA.jpg|50px]] <!-- File:Ariel (moon).jpg -->
|bgcolor=black|[[File:Ariel-NASA.jpg|50px]]
|578.9
|578.9
|0.091
|0.091
Line 544: Line 544:
|-
|-
|[[Ceres (dwarf planet)|Ceres]]<sup>‡</sup> <br><small> 1</small>
|[[Ceres (dwarf planet)|Ceres]]<sup>‡</sup> <br><small> 1</small>
|bgcolor=black|[[File:Ceres_optimized.jpg|50px]]
|bgcolor=black|[[File:Ceres optimized.jpg|50px]]
|475
|475
|0.076
|0.076
Line 560: Line 560:
|bgcolor=black|[[File:Quaoar PRC2002-17e.jpg|50px]]
|bgcolor=black|[[File:Quaoar PRC2002-17e.jpg|50px]]
|445<ref name=Brown2010>{{cite journal
|445<ref name=Brown2010>{{cite journal
|last=Brown |first=Michael E.
|last=Brown |first=Michael E.
|coauthors=Fraser, Wesley C.
|coauthors=Fraser, Wesley C.
|title=Quaoar: A Rock in the Kuiper belt
|title=Quaoar: A Rock in the Kuiper belt
|journal=The Astrophysical Journal
|journal=The Astrophysical Journal
|volume= 714|issue= 2|pages= 1547|year=2010
|volume= 714|issue= 2|pages= 1547|year=2010
|arxiv=1003.5911
|arxiv=1003.5911
|bibcode = 2010ApJ...714.1547F
|bibcode = 2010ApJ...714.1547F
|doi=10.1088/0004-637X/714/2/1547
|doi=10.1088/0004-637X/714/2/1547
}}</ref>
}}</ref>
| 0.07
| 0.07
Line 816: Line 816:
|colspan="8"|
|colspan="8"|
|[[Detached object]]<ref name=Buie10KZ39>{{cite web
|[[Detached object]]<ref name=Buie10KZ39>{{cite web
|author=[[Marc W. Buie]]
|author=[[Marc W. Buie]]
|date=2010-06-16 using 19 of 19 observations over 0.98 years (356 days)
|date=2010-06-16 using 19 of 19 observations over 0.98 years (356 days)
|title=Orbit Fit and Astrometric record for 10KZ39
|title=Orbit Fit and Astrometric record for 10KZ39
|publisher=SwRI (Space Science Department)
|publisher=SwRI (Space Science Department)
|url=http://www.boulder.swri.edu/~buie/kbo/astrom/10KZ39.html
|url=http://www.boulder.swri.edu/~buie/kbo/astrom/10KZ39.html
|accessdate=2011-08-18}}</ref> or [[Classical Kuiper belt object|Cubewano]]<ref name=MPC10KZ39>{{cite web
|accessdate=2011-08-18}}</ref> or [[Classical Kuiper belt object|Cubewano]]<ref name=MPC10KZ39>{{cite web
|title=2010 KZ39
|title=2010 KZ39
|publisher=IAU Minor Planet Center
|publisher=IAU Minor Planet Center
|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=2010+KZ39&commit=Show
|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=2010+KZ39&commit=Show
|accessdate=2011-08-18}}</ref>
|accessdate=2011-08-18}}</ref>
|unknown
|unknown
|-
|-
Line 986: Line 986:
! class="unsortable" | Volume<br><small>(V<sub>⊕</sub>)</small>
! class="unsortable" | Volume<br><small>(V<sub>⊕</sub>)</small>
! Mass<br><small>{{e|21}}&nbsp;kg <br> ([[Yottagram|Yg]]) </small>
! Mass<br><small>{{e|21}}&nbsp;kg <br> ([[Yottagram|Yg]]) </small>
! class="unsortable" | Mass<br><small>(M<sub>⊕</sub>)</small>
! class="unsortable" | Mass<br><small>(M<sub>⊕</sub>)</small>
! Density<ref>Densities of those KBOs whose masses are uncertain are assumed to be 2.0 in line with Pluto</ref><br><small>g/cm<sup>3</sup></small>
! Density<ref>Densities of those KBOs whose masses are uncertain are assumed to be 2.0 in line with Pluto</ref><br><small>g/cm<sup>3</sup></small>
! Surface gravity <br> (m/s<sup>2</sup>)
! Surface gravity <br> (m/s<sup>2</sup>)
Line 1,047: Line 1,047:
|unknown
|unknown
|-
|-
|{{mpl|2004 XR|190}} <br><small> "Buffy"</small>
|{{mpl|2004 XR|190}} <br><small> "Buffy"</small>
|bgcolor=black|
|bgcolor=black|
|277<ref name="johnston2010">{{cite web
|277<ref name="johnston2010">{{cite web
Line 1,096: Line 1,096:
|-
|-
|[[2 Pallas|Pallas]]<sup>$</sup> <br><small> 2</small>
|[[2 Pallas|Pallas]]<sup>$</sup> <br><small> 2</small>
|bgcolor=black|[[File:PallasHST2007.jpg|50px|]]
|bgcolor=black|[[File:PallasHST2007.jpg|50px| ]]
|266<ref>{{cite web|author=Alan Chamberlin |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2;orb=0;cov=0;log=0;cad=0#phys_par |title=JPL Small-Body Database Browser |publisher=Ssd.jpl.nasa.gov |date= |accessdate=2011-01-04|archiveurl = http://www.webcitation.org/5wRXdqRMp |archivedate = 2011-02-12|deadurl=no}}</ref>
|266<ref>{{cite web|author=Alan Chamberlin |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2;orb=0;cov=0;log=0;cad=0#phys_par |title=JPL Small-Body Database Browser |publisher=Ssd.jpl.nasa.gov |date= |accessdate=2011-01-04|archiveurl = http://www.webcitation.org/5wRXdqRMp |archivedate = 2011-02-12|deadurl=no}}</ref>
|0.042
|0.042
Line 1,482: Line 1,482:
|[[(145480) 2005 TB190|(145480) 2005 TB<sub>190</sub>]]
|[[(145480) 2005 TB190|(145480) 2005 TB<sub>190</sub>]]
|bgcolor=black|
|bgcolor=black|
|186.25 <!-- Muller2010 (335-410 diameter) --><ref name=autogenerated2>{{cite journal|last=Muller|first=T.G.|coauthors=Lellouch, E.; Stansberry, J. ''et al.''|title="TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)|journal=Astronomy and Astrophysics|volume=518|year=2010|page=L146|doi=10.1051/0004-6361/201014683|bibcode=2010A&A...518L.146M|url=http://adsabs.harvard.edu/abs/2010A%26A...518L.146M|archiveurl = http://www.webcitation.org/5wRXdDjxM |archivedate = 2011-02-12|deadurl=no}}</ref>
|186.25 <!-- Muller2010 (335-410 diameter) --><ref name=autogenerated2>{{cite journal|last=Muller|first=T.G.|coauthors=Lellouch, E.; Stansberry, J. ''et al.''|title="TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)|journal=Astronomy and Astrophysics|volume=518|year=2010|page=L146|doi=10.1051/0004-6361/201014683|bibcode=2010A&A...518L.146M|url=http://adsabs.harvard.edu/abs/2010A%26A...518L.146M|archiveurl = http://www.webcitation.org/5wRXdDjxM |archivedate = 2011-02-12|deadurl=no}}</ref>
| <!-- |0.039
| <!-- |0.039
|0.065
|0.065
Line 1,490: Line 1,490:
|2.0
|2.0
|{{Gr|0.13|250}}
|{{Gr|0.13|250}}
|0.014 for 250&nbsp;km radius -->
|0.014 for 250&nbsp;km radius -->
|[[Detached object]]
|[[Detached object]]
|unknown
|unknown
Line 1,588: Line 1,588:
|bgcolor=black|[[File:TX300-2009Nov16-04UT.jpg|50px]]
|bgcolor=black|[[File:TX300-2009Nov16-04UT.jpg|50px]]
|143<!--286/2 = 143--><ref name="msnbc55636">{{cite web
|143<!--286/2 = 143--><ref name="msnbc55636">{{cite web
|date=2010-06-16
|date=2010-06-16
|title=Scientists size up a bright mini-world
|title=Scientists size up a bright mini-world
|publisher=MSNBC
|publisher=MSNBC
|author=Clara Moskowitz
|author=Clara Moskowitz
|url=http://www.msnbc.msn.com/id/37735465/ns/technology_and_science-space/
|url=http://www.msnbc.msn.com/id/37735465/ns/technology_and_science-space/
|accessdate=2010-06-16}}</ref>
|accessdate=2010-06-16}}</ref>
|12 <!-- assumed value from wiki page-->
|12 <!-- assumed value from wiki page-->
|[[Kuiper belt object]]—[[Haumea family]]
|[[Kuiper belt object]]—[[Haumea family]]
Line 1,647: Line 1,647:
|title=JPL Small-Body Database Browser: 65 Cybele
|title=JPL Small-Body Database Browser: 65 Cybele
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=65
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=65
|accessdate=2008-11-25| archiveurl = http://www.webcitation.org/5mqpk4wfX |archivedate = 2010-01-17| deadurl=no}}</ref> <small>IRAS</small>
|accessdate=2008-11-25| archiveurl = http://www.webcitation.org/5mqpk4wfX |archivedate = 2010-01-17| deadurl=no}}</ref> <small>IRAS</small>
|17.8
|17.8
|Outer [[main-belt asteroid]]{{mdash}}[[C-type asteroid|C-type]]
|Outer [[main-belt asteroid]]{{mdash}}[[C-type asteroid|C-type]]
Line 1,820: Line 1,820:
|url=http://web.media.mit.edu/~win/hstpub.pdf
|url=http://web.media.mit.edu/~win/hstpub.pdf
|accessdate=2005-01-15
|accessdate=2005-01-15
|doi=10.1006/icar.1999.6047 |bibcode=1999Icar..137..260S}} {{Dead link|date=October 2010|bot=H3llBot}}</ref> <!-- old 103.9-->
|doi=10.1006/icar.1999.6047 |bibcode=1999Icar..137..260S}} {{Dead link|date=October 2010|bot=H3llBot}}</ref> <!-- old 103.9-->
|12.7
|12.7
|[[Main-belt asteroid]]{{mdash}}[[G-type asteroid|G-type]]
|[[Main-belt asteroid]]{{mdash}}[[G-type asteroid|G-type]]
Line 1,950: Line 1,950:


===Selected objects between 100 and 50&nbsp;km in radius===
===Selected objects between 100 and 50&nbsp;km in radius===
Objects 100 and 50&nbsp;km in radius (200&nbsp;km to 100&nbsp;km in average diameter). This currently includes most objects in the [[asteroid belt]] and moons of the [[gas giants]] in this size range, but is missing many newly discovered objects in the outer Solar System such as here.<ref name="johnstonsarchive1"/> [[Asteroid spectral types]] are mostly Tholen, but some might be SMASS.
Objects 100 and 50&nbsp;km in radius (200&nbsp;km to 100&nbsp;km in average diameter). This currently includes most objects in the [[asteroid belt]] and moons of the [[gas giants]] in this size range, but is missing many newly discovered objects in the outer Solar System such as here.<ref name="johnstonsarchive1"/> [[Asteroid spectral types]] are mostly Tholen, but some might be SMASS.


{| class="wikitable sortable"
{| class="wikitable sortable"
Line 1,970: Line 1,970:
|[[Main-belt asteroid]]{{mdash}}[[S-type asteroid|S-type]]
|[[Main-belt asteroid]]{{mdash}}[[S-type asteroid|S-type]]
|-
|-
| [[24 Themis]] <sup>M</sup>
| [[24 Themis]] <sup>M</sup>
|bgcolor=black|
|bgcolor=black|
|99
|99
Line 2,024: Line 2,024:
|[[Main-belt asteroid]]{{mdash}}[[M-type asteroid|M-type]]
|[[Main-belt asteroid]]{{mdash}}[[M-type asteroid|M-type]]
|-
|-
|[[6 Hebe]] <sup>$</sup>
|[[6 Hebe]] <sup>$</sup>
|bgcolor=black|
|bgcolor=black|
|92.59<ref name=PSI/> <!-- old: 93.1-->
|92.59<ref name=PSI/> <!-- old: 93.1-->
Line 2,134: Line 2,134:
|issue=1
|issue=1
|page=286
|page=286
|bibcode=2007Icar..191..286G}}</ref> <!-- old data 229.7 / 2 = 114.85 <ref name=spitzer/> -->
|bibcode=2007Icar..191..286G}}</ref> <!-- old data 229.7 / 2 = 114.85 <ref name=spitzer/> -->
|5.4<ref name="Grundy2007"/>
|5.4<ref name="Grundy2007"/>
|[[Centaur (minor planet)|Centaur]]{{mdash}}[[Trans-Neptunian object|TNO]]{{mdash}}[[Minor planet moon|binary]]
|[[Centaur (minor planet)|Centaur]]{{mdash}}[[Trans-Neptunian object|TNO]]{{mdash}}[[Minor planet moon|binary]]
Line 4,403: Line 4,403:
| [[2000 Herschel]]
| [[2000 Herschel]]
|bgcolor=black|
|bgcolor=black|
| 8<ref>[http://asteroidoccultation.com/2011_08/0826_2000_24820_Summary.txt IOTA/IOTA-ES occultation update for (2000) Herschel]</ref>
| 8<ref>[http://asteroidoccultation.com/2011_08/0826_2000_24820_Summary.txt IOTA/IOTA-ES occultation update for (2000) Herschel]</ref>
|
|
|[[Main-belt asteroid]]<ref>[http://ssd.jpl.nasa.gov/sbdb.cgi?ID=a0002000 JPL Small-Body Database Browser: 2000 Herschel]</ref>
|[[Main-belt asteroid]]<ref>[http://ssd.jpl.nasa.gov/sbdb.cgi?ID=a0002000 JPL Small-Body Database Browser: 2000 Herschel]</ref>
Line 4,488: Line 4,488:
|bgcolor=black|
|bgcolor=black|
|5.0<ref name=sheppard>{{cite web
|5.0<ref name=sheppard>{{cite web
|title=Uranus' Known Satellites
|title=Uranus' Known Satellites
|publisher=Carnegie Institution (Department of Terrestrial Magnetism)
|publisher=Carnegie Institution (Department of Terrestrial Magnetism)
|author=[[Scott S. Sheppard]]
|author=[[Scott S. Sheppard]]
|url=http://www.dtm.ciw.edu/users/sheppard/satellites/urasatdata.html
|url=http://www.dtm.ciw.edu/users/sheppard/satellites/urasatdata.html
|accessdate=2011-01-22}}</ref>
|accessdate=2011-01-22}}</ref>
|
|
|[[Moons of Uranus|Satellite of Uranus]]
|[[Moons of Uranus|Satellite of Uranus]]
Line 4,695: Line 4,695:
|-
|-
|[[2867 Šteins]]
|[[2867 Šteins]]
|bgcolor=black| [[File:Steins-Rosetta.jpg|50px|center]]
|bgcolor=black|
|2.65<!--5.3&nbsp;km mean diameter--><ref name="keller">[http://www.sciencemag.org/cgi/content/abstract/327/5962/190http://www.sciencemag.org/cgi/content/abstract/327/5962/190 H. U. Keller, et all - '''E-Type Asteroid (2867) Steins as Imaged by OSIRIS on Board Rosetta''' - Science 8 January 2010: Vol. 327. no. 5962, pp. 190 - 193 DOI: 10.1126/science.1179559] {{dead link|date=February 2011}}</ref>
|2.65<!--5.3&nbsp;km mean diameter--><ref name="keller">[http://www.sciencemag.org/cgi/content/abstract/327/5962/190http://www.sciencemag.org/cgi/content/abstract/327/5962/190 H. U. Keller, et all - '''E-Type Asteroid (2867) Steins as Imaged by OSIRIS on Board Rosetta''' - Science 8 January 2010: Vol. 327. no. 5962, pp. 190 - 193 DOI: 10.1126/science.1179559] {{dead link|date=February 2011}}</ref>
|
|
Line 5,030: Line 5,030:
|≈800<ref>[http://www.spaceref.com/news/viewpr.html?pid=23753 Minor Planet No. 100,000 Named for Space Age 50th Anniversary (2007) - Space Ref, Quote: "..about a mile in size"]</ref>
|≈800<ref>[http://www.spaceref.com/news/viewpr.html?pid=23753 Minor Planet No. 100,000 Named for Space Age 50th Anniversary (2007) - Space Ref, Quote: "..about a mile in size"]</ref>
|
|
|Inner Main-belt Asteroid<ref>[JPL Small-Body Database Browser: 100000 Astronautica]</ref>
|Inner Main-belt Asteroid<ref>[JPL Small-Body Database Browser: 100000 Astronautica]</ref>
|-
|-
|[[Dactyl (moon)|Dactyl]]<br><sup>Ida I</sup>
|[[Dactyl (moon)|Dactyl]]<br><sup>Ida I</sup>
Line 5,128: Line 5,128:
|-
|-
|[[6489 Golevka]]
|[[6489 Golevka]]
|bgcolor=black| <!-- radar to CGI -->
|bgcolor=black| <!-- radar to CGI -->
|350<ref>{{cite web|author=Alan Chamberlin |url=http://ssd.jpl.nasa.gov/sbdb.cgi#top |title=JPL Small-Body Database Browser |publisher=Ssd.jpl.nasa.gov |date= |accessdate=2011-01-04|archiveurl = http://www.webcitation.org/5wRY4Rkg7 |archivedate = 2011-02-12|deadurl=no}}</ref>
|350<ref>{{cite web|author=Alan Chamberlin |url=http://ssd.jpl.nasa.gov/sbdb.cgi#top |title=JPL Small-Body Database Browser |publisher=Ssd.jpl.nasa.gov |date= |accessdate=2011-01-04|archiveurl = http://www.webcitation.org/5wRY4Rkg7 |archivedate = 2011-02-12|deadurl=no}}</ref>
|
|
Line 5,134: Line 5,134:
|-
|-
|[[25143 Itokawa]]
|[[25143 Itokawa]]
|bgcolor=black|<!-- [[File:Itokawa4.jpg|50px]] not GPL -->
|bgcolor=black|
| 346
| 346
|0.0358
|0.0358
Line 5,163: Line 5,163:
|[[Near-Earth asteroid]]{{mdash}}[[Apollo asteroid|Apollo]]
|[[Near-Earth asteroid]]{{mdash}}[[Apollo asteroid|Apollo]]
|-
|-
|[[2005 YU55]] <ref>[http://www.bbc.co.uk/news/science-environment-15572634 BBC - '''Giant asteroid passes near Earth''' - 9 November 2011]</ref>
|[[2005 YU55]] <ref>[http://www.bbc.co.uk/news/science-environment-15572634 BBC - '''Giant asteroid passes near Earth''' - 9 November 2011]</ref>
|bgcolor=black|[[File:2005YU55-20111107.jpg|50px|center]] <!-- radar image -->
|bgcolor=black|[[File:2005YU55-20111107.jpg|50px|center]]
|155-170<ref>[http://www.mpg.de/4652308/2005_YU55_rocks_in_space?filter_order=L The Herschel Space Observatory catches a glimpse of the minor planet during its rendezvous with Earth (November 17, 2011)]</ref>
|155-170<ref>[http://www.mpg.de/4652308/2005_YU55_rocks_in_space?filter_order=L The Herschel Space Observatory catches a glimpse of the minor planet during its rendezvous with Earth (November 17, 2011)]</ref>
|
|
Line 5,276: Line 5,276:
| [[File:Callisto.jpg|center|100x100px]]
| [[File:Callisto.jpg|center|100x100px]]
| [[File:Io highest resolution true color.jpg|center|100x100px]]
| [[File:Io highest resolution true color.jpg|center|100x100px]]
| [[File:Cara-oculta-luna.jpg|center|100x100px]] <!-- File:Full Moon Luc Viatour.jpg -->
| [[File:Cara-oculta-luna.jpg|center|100x100px]]
|-
|-
| '''[[Mars]]'''
| '''[[Mars]]'''
Line 5,289: Line 5,289:
| [[File:Triton moon mosaic Voyager 2 (large).jpg|center|100x100px]]
| [[File:Triton moon mosaic Voyager 2 (large).jpg|center|100x100px]]
| [[File:Titania (moon) color cropped.jpg|center|110x110px]]
| [[File:Titania (moon) color cropped.jpg|center|110x110px]]
| [[File:PIA08148 (Rhea-Splat).jpg|center|100x100px]] <!-- File:Rhea hi-res PIA07763.jpg -->
| [[File:PIA08148 (Rhea-Splat).jpg|center|100x100px]]
| [[File:Voyager 2 picture of Oberon.jpg|center|100x100px]]
| [[File:Voyager 2 picture of Oberon.jpg|center|100x100px]]
| [[File:Iapetus as seen by the Cassini probe - 20071008.jpg|center|100x100px]]
| [[File:Iapetus as seen by the Cassini probe - 20071008.jpg|center|100x100px]]
Line 5,303: Line 5,303:
|-style="background: Black;"
|-style="background: Black;"
| [[File:Ariel-NASA.jpg|center|100x100px]]
| [[File:Ariel-NASA.jpg|center|100x100px]]
| [[File:Dionean Linea PIA08256.jpg|center|100x100px]] <!-- File:PIA09861.jpg File:Dione (Mond) (30823363).jpg -->
| [[File:Dionean Linea PIA08256.jpg|center|100x100px]]
| [[File:Inset-sat tethys-large.jpg|center|100x100px]]
| [[File:Inset-sat tethys-large.jpg|center|100x100px]]
| [[File:Vesta from Dawn, July 17.jpg|center|100x100px]] <!-- File:Dawn-image-070911.jpg -->
| [[File:Vesta from Dawn, July 17.jpg|center|100x100px]]
| [[File:Enceladus from Voyager.jpg|center|100x100px]]
| [[File:Enceladus from Voyager.jpg|center|100x100px]]
| [[File:Miranda.jpg|center|100x100px]]
| [[File:Miranda.jpg|center|100x100px]]
Line 5,318: Line 5,318:
| '''[[Proteus (moon)|Proteus]]'''
| '''[[Proteus (moon)|Proteus]]'''
|-style="background: Black;"
|-style="background: Black;"
| [[File:Mimas before limb sharp (colored).jpg|center|100x100px]] <!-- File:Mimas moon.jpg -->
| [[File:Mimas before limb sharp (colored).jpg|center|100x100px]]
| [[File:Hyperion in natural colours.jpg|center|100x100px]]
| [[File:Hyperion in natural colours.jpg|center|100x100px]]
| [[File:Phoebe cassini.jpg|center|100x100px]]
| [[File:Phoebe cassini.jpg|center|100x100px]]

Revision as of 02:20, 25 December 2011

Template:Lists of Solar System objects

The image is of the masses of the heaviest objects

This is a list of Solar System objects by size, arranged in descending order of mean volumetric radius. The list can also be partially sorted according to an object's mass and, for the largest objects, volume, density and surface gravity. This list contains the Sun, the planets, (candidate) dwarf planets, many of the larger small Solar System bodies (which includes the asteroids), all named natural satellites, and a number of smaller objects of historical or scientific interest, such as comets and near-Earth objects.

The ordering may be different depending on whether one chooses radius or mass, because some objects are denser than others. For instance Uranus is bigger than Neptune but less massive, and although Ganymede and Titan are larger than Mercury, they have less than half its mass. This means some objects in the lower tables, despite their smaller radii, may be more massive than objects in the upper tables because they have a higher density.

Many trans-Neptunian objects (TNOs) have been discovered, and their approximate locations in this list are shown, even though there can be a large uncertainty in their measurement.

Solar System objects more massive than 1021 kilograms (one yottagram [Yg]) are known or expected to be approximately spherical. Astronomical bodies relax into rounded shapes (ellipsoids), achieving hydrostatic equilibrium, when the gravity of their mass is sufficient to overcome the structural strength of their material. These are dubbed "regular". Objects made of ice become regular more easily than those made of rock, and many icy objects are spheroidal at far lower sizes. The cutoff boundary for regularity is somewhere between 100 km and 200 km in radius.[1]

The larger objects in the mass range between 1018 kg to 1021 kg (1 to 1000 zettagrams (Zg)) such as Tethys, Ceres, and Mimas, have relaxed to an equilibrium oblate spheroid due to their gravity, while the less massive rubble piles (e.g. Amalthea and Janus) are roughly rounded, but not spherical, dubbed "irregular".

Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation, but a characteristic feature of the "irregular"-shaped bodies is that there is a significant difference in the length of their two equatorial diameters.

There can be difficulty in figuring out the diameter (within a factor of about 2) for typical objects beyond Saturn. (See 2060 Chiron as an example.) For TNOs there is some confidence in the diameters, but for non-binary TNOs there is no real confidence in the "unreferenced wiki-assumed" masses/densities. Many TNOs are just assumed to have a density of 2.0 g/cm3, though it is just as likely that they have a comet-like density of only 0.5 g/cm3.[2] Thus most provisional TNOs are not given an MEarth value to prevent from cluttering the list with too many assumptions that could be off by an order of magnitude. For example, if a TNO is poorly assumed to have a mass of 3.59×1020 kg based on a radius of 350 km with a density of 2 g/cm3 and is later discovered to only have a radius of 175 km with a density of 1 g/cm3, the mass estimate would be only 2.24×1019 kg.

The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters. But many of the moons with a radius less than ~100 km, such as Jupiter's Himalia, still have unknown masses with assumed densities.[3] Again, as we get further from the Sun than Saturn, things get less clear. There has not yet been an orbiter around Uranus or Neptune for long-term study of the moons. For the small outer irregular moons of Uranus, such as Sycorax, which were not discovered by the Voyager 2 flyby, even different NASA web pages, such as the National Space Science Data Center[4] and JPL Solar System Dynamics,[3] have somewhat contradictory size and albedo estimates depending on which research paper is being cited.

Data for objects has varying reliability including uncertainties in the figures for mass and radius, and irregularities in the shape and density, with accuracy often depending on how close it is to Earth or if it has been visited by a probe.

List

Objects above ≈300 km in radius

Anything above this size is probably in hydrostatic equilibrium, but some bodies near the end of this list may not. However, their predicted or measured size would need to be "grossly in error" or their composition primarily rocky, for them not to be.[5] A lot of the values are manually calculated assuming sphericity. Size may or may not include an object's atmosphere. The diameter of Saturn's rings is around 364,900 km, much wider than Jupiter, but its gaseous sphere is smaller.

Body Image Mean radius
(km)
Mean radius
(R)
Volume
(109 km3)
Volume
(V)
Mass
×1021 kg
(Yg)
Mass
(M)
Density[6]
g/cm3
Surface gravity
(m/s2)
Surface gravity
(⊕)
Type of object Shape
Sun 696,000 109.25 1,412,000,000 1,303,781 1,989,100,000 332,837 1.409 274.0 28.02 Star regular
Jupiter 69,911 10.97 1,431,280 1,321 1,898,600 317.83 1.33 24.79 2.535 Planet (gas giant) regular
Saturn 58,232
(w/o rings)
9.14 827,130 764 568,460 95.159 0.70 10.445 1.06 Planet (gas giant) regular
Uranus 25,362 3.98 68,340 63.1 86,832 14.536 1.30 8.87 0.90 Planet (gas giant) regular
Neptune 24,622 3.86 62,540 57.7 102,430 17.147 1.76 11.15 1.140 Planet (gas giant) regular
Earth 6,371.0 1 1,083.21 1 5,973.6 1 5.515 9.78033 1 Planet (terrestrial) regular
Venus 6,051.8
(w/o gas)
0.950 928.43 0.857 4,868.5 0.815 5.24 8.872 0.91 Planet (terrestrial) regular
Mars 3,390.0 0.532 163.18 0.151 641.85 0.107 3.94 3.7 0.38 Planet (terrestrial) regular
Ganymede
Jupiter III
2,631.2 0.413 76.30 0.0704 148.2 0.0248 1.936 1.428 0.15 Satellite of Jupiter regular
Titan
Saturn VI
2,576[7]
(w/o gas)
0.404 71.52 0.0660 134.5 0.0225 1.88 1.354 0.14 Satellite of Saturn regular
Mercury 2,439.7 0.383 60.83 0.0562 330.2 0.0553 5.43 3.7 0.38 Planet (terrestrial) regular
Callisto
Jupiter IV
2,410.3 0.378 58.65 0.0541 107.6 0.018 1.83 1.23603 0.126 Satellite of Jupiter regular
Io
Jupiter I
1,821.5 0.286 25.32 0.0234 89.3 0.015 3.528 1.797 0.183 Satellite of Jupiter regular
Moon 1,737.1 0.273 21.958 0.0203 73.5 0.0123 3.3464 1.625 0.166 Satellite of Earth regular
Europa
Jupiter II
1,561 0.245 15.93 0.0147 48 0.00803 3.01 1.316 0.134 Satellite of Jupiter regular
Triton
Neptune I
1,353.4 0.212 10.38 0.0096 21.5 0.00359 2.061 0.782 0.0797 Satellite of Neptune regular
ErisR
136199
1,163[8] 0.182 7 0.007 16.7[9] 0.0027 2.25 0.659 0.0677 Dwarf planetSDObinary regular
PlutoR
134340
1,161[10]
(w/o gas)
0.181 7.15 0.0066 13.105 0.0022 2.0 0.61 0.062 Dwarf planet
KBO
regular
Titania
Uranus III
788.9 0.124 2.06 0.0019 3.526 0.00059 1.72 0.378 0.0385 Satellite of Uranus regular
Rhea
Saturn V
764.1[11] 0.12 1.87 0.0017 2.3166 0.00039 1.23 0.26 0.027 Satellite of Saturn regular
Oberon
Uranus IV
761.4 0.12 1.85 0.0017 3.014 0.0005 1.63 0.347 0.035 Satellite of Uranus regular
Iapetus
Saturn VIII
735.6[12] 0.113 1.55 0.0014 1.9739 0.00033 1.08 0.223 0.0227 Satellite of Saturn regular
MakemakeRA
136472
710[13] 0.126
–0.157
1.8 0.002 3 0.00067 2.0 0.4 0.04 Dwarf planet
KBO
regular
Charon
Pluto I
603.5[14] 0.095 0.87 0.0008 1.52 0.00025 1.65 0.279 0.028 Satellite of Pluto regular
SednaRA
90377
600–800[15] 0.09
–0.14
1.73 0.0016 3 0.00050 2.0 0.33
–0.50
0.0337
–0.0511
Detached object unknown
2007 OR10
225088
"Snow White"
≈600[16]–710[5] 0.094 0.904 0.0008 1.81P 0.0003 2.0P 0.168 0.017 SDO unknown
Umbriel
Uranus II
584.7 0.092 0.84 0.0008 1.2 0.00020 1.4 0.234 0.024 Satellite of Uranus regular
Ariel
Uranus I
File:Ariel-NASA.jpg 578.9 0.091 0.81 0.0008 1.35 0.00022 1.67 0.269 0.027 Satellite of Uranus regular
HaumeaR
136108
File:2003 EL61.jpg 575[17]–750[5] 0.117 1.3–1.6 0.001 4.006 0.00069 2.551[18] 0.44 0.045 Dwarf planet
KBOtrinary
regular (scalene ellipsoid)
Dione
Saturn IV
561.6 0.088 0.73 0.0007 1.096 0.000183 1.48 0.232 0.0236 Satellite of Saturn regular
Tethys
Saturn III
533 0.083 0.624 0.0006 0.6173 0.000103 1.15 0.145 0.015 Satellite of Saturn regular
Ceres
1
475 0.076 0.437 0.0004 0.95 0.000159 2.08 0.27 0.0275 Dwarf planetAsteroid regular
Quaoar
50000
445[19] 0.07 0.37 0.0003 1.6[19] 0.0003 4.2[19] 0.125 0.013 KBOCubewanobinary unknown
OrcusRA
90482
425[13] 0.069
–0.08
0.4 0.0004 0.63A 0.0001 1.5 0.233 0.023 KBOPlutinobinary unknown
2002 TC302R
84522
410–570[20] 0.09 0.786 0.0007 1.573P 0.00026 2.0 0.32 0.033 KBO2:5 resonance unknown
2007 UK1269
229762
File:MinorPlanet-2007uk126-19970930.gif 375[5] 0.069 0.354 0.0003 0.708P 0.0001 2.0 0.245 0.025 SDO unknown
2005 UQ5139
202421
375[5] 0.074 0.443 0.0004 0.886P 0.0001 2.0 0.277 0.0284 KBOCubewano unknown
2003 MW129
174567
375[5] 0.0658 0.308 0.0003 0.616P 0.0001 2.0 0.228 0.02 KBO unknown
2002 AW197R
55565
370[5] 0.0576 0.207 0.00019 0.414P 0.000069 2.0 0.205 0.0211 KBO[21] unknown
2005 QU1829
303775
365[5] 0.082 0.606 0.00056 1.21P 0.0002 2.0 0.293 0.03 SDO[22] unknown
2002 MS4 360[5]R 0.057 0.203 0.00018 0.4005P 0.000067 2.0P 0.203 0.02086 KBO[21] unknown
2007 JJ43
278361
350[5] TNO[21] unknown
2003 AZ84R
208996
345[5] 0.0538 0.169 0.000156 0.53P 5.66 E-5 2.0P 0.171 0.02 KBOPlutinobinary unknown
2010 EK139 340[5] SDO unknown
2002 UX25R
55637
340[5] 0.0535 0.166 0.000153 0.331P 0.0000554 2.0 0.19 0.01952 KBObinary unknown
2004 GV9R
90568
340[5] 0.0531 0.162 0.00015 0.325P 0.0000534 2.0 0.189 0.0194 KBO unknown
2006 QH1819 340[5] 0.06 0.233 0.000215 0.467P 0.00008 2.0 0.214 0.022 SDO unknown
2005 RN439
145452
330[5] 0.0573 0.2036 0.00019 0.407P 0.000068 2.0 0.204 0.02096 KBO[21] unknown
2010 KZ39 330[5] Detached object[23] or Cubewano[24] unknown
IxionRA
28978
Template:Listrow KBO unknown
2004 XA192
230965
320[5] 0.055 0.177 0.00016 0.354P 0.000059 2.0 0.195 0.02 TNO[21] unknown
2003 VS2
84922
315[5] 0.057 0.203 0.00018 0.4005P 0.000067 2.0 0.203 0.02086 KBOPlutino[21] unknown
2001 UR1639
42301
305[5] 0.05 0.134 0.00012 0.269P 0.000045 2.0P 0.178 0.018 SDO[21] unknown
Salacia
120347
305[5] 0.0455 0.102 0.00009 0.2P 0.000034 2.0P 0.159 0.016 KBObinary unknown
2010 RE64 305[5] KBO unknown
2010 RF43 305[5] SDO unknown
2004 PF115
175113
305[5] KBOPlutino unknown
2003 UZ4139 300[5] 0.048 0.116 0.00012 0.33P 0.000055 2.0P 0.24 0.0246 KBOPlutino unknown
2008 ST291 300[5] SDO unknown
2010 FX86 300[5] KBOCubewano unknown

Selected objects between ≈300 and ≈200 km in radius

Satellites in this size range tend to be round (although Proteus is not), and TNOs are expected to be as well, assuming the estimated size is correct. The asteroid 10 Hygiea is not, and 2 Pallas and 4 Vesta are borderline.

Body Image Mean radius
(km)
Mean radius
(R)
Volume
(109 km3)
Volume
(V)
Mass
×1021 kg
(Yg)
Mass
(M)
Density[25]
g/cm3
Surface gravity
(m/s2)
Surface gravity
(⊕)
Type of object Shape
2005 RM439
145451
290[26] 0.0455 0.102 0.00009 0.2P 0.000034 2.0P 0.159 0.016 KBO unknown
2004 NT33 290[21] 0.043 0.089 0.000082 0.178P 0.000029 2.0P 0.155 0.0158 KBOCubewano[21] unknown
1996 TL66RA
15874
Template:Listrow[5] SDO unknown
2004 UX10
144897
284.5[5] 0.039 0.065 0.00006 0.13P 0.000022 2.0P 0.139 0.014 KBO unknown
2004 XR190
"Buffy"
277[21]* 0.059 0.221 0.0002 0.4416P 0.00007 2.0P 0.21 0.0215 SDO[21] unknown
2004 TY364*
120348
277[21] 0.043 0.089 0.000082 0.178P 0.000029 2.0P 0.155 0.0158 KBO[21] unknown
HuyaR
38628
266[20] 0.04175 0.0788 0.000073 0.158P 0.00026 2.0P 0.149 0.015 KBOPlutino unknown
Pallas$
2
266[27] 0.042 0.078 0.00007 0.211 0.0000353 2.8[28] 0.199 0.02 Asteroid uncertain
Vesta$
4
264.6 0.042 0.078 0.00007 0.262 0.0000438 3.42[29] 0.25 0.0256 Asteroid regular?
2004 PR107 264.5[21] 0.0345 0.0446 0.00004 0.089P 0.000014 2.0P 0.123 0.0126 KBO unknown
2003 QX113 252.5[21] 0.036 0.051 0.00005 0.102P 0.000017 2.0P 0.129 0.013 SDO[21] unknown
Enceladus
Saturn II
252.1 0.039 0.067 0.00006 0.108 0.0000181 1.61 0.111 0.0113 Satellite of Saturn regular
Varuna*
20000
250[5]–530 0.049 0.125 0.000115 0.37 6.2E-5 0.992[18] 0.258 0.028 KBO unknown
2006 HH123 239[5] 0.031 0.0335 0.000011 0.067P 0.000011 2.0 0.112 0.011 Centaur[21] unknown
Miranda
Uranus V
235.8 0.037 0.055 0.00005 0.0659 0.000011 1.20 0.0791 0.00806 Satellite of Uranus regular
1999 DE9
26375
230.5[20] 0.036 0.051 0.000047 0.1026P 0.000017 2.0 0.129 0.013 KBO unknown
Chaos*
19521
230–372.5[22] 0.0585 0.216 0.0002 0.4328P 0.00007 2.0P 0.208 0.021 KBOCubewano unknown
1998 SN165*
35671
230[26] 0.036 0.05 0.000046 0.1P 0.000017 2.0 0.127 0.013 KBO unknown
2002 XV93 220[21] 0.036 0.051 0.00005 0.102P 0.000017 2.0 0.129 0.013 Plutino[21] unknown
2003 FY128*
120132
220[21] 0.0345 0.0446 0.00004 0.089P 0.000014 2.0 0.123 0.0126 SDO[21] unknown
2000 YW134*
82075
215.5[21] 0.039 0.065 0.00006 0.13P 0.000022 2.0P 0.139 0.014 SDO[21] unknown
1999 CD158 210[21] 0.0345 0.0446 0.00004 0.089P 0.000014 2.0 0.123 0.0126 KBO unknown
Proteus A
Neptune VIII (8)
210 0.033 0.038 0.000035 0.050 0.00000844 1.3[30] 0.0666 0.00678 Satellite of Neptune irregular
2001 QF298 210[21]* 0.04 0.067 0.00006 0.134P 0.000022 2.0 0.141 0.014 Plutino[21] unknown
10 Hygiea$ Template:Listrow Asteroid irregular
2002 WC19
119979
200.5[31] 0.0315 0.034 0.00003 0.0675P 0.000011 2.0 0.112 0.0115 KBObinary unknown
1996 GQ21*
26181
200.5[21] 0.031 0.0335 0.000011 0.067P 0.000011 2.0 0.112 0.011 SDO[21] unknown
Mimas
Saturn I
198.3 0.031 0.033 0.00003 0.03749 0.0000063 1.15 0.06363 0.00648 Satellite of Saturn regular

Selected objects between 200 and 100 km in radius

Objects between 200 and 100 km in radius (400 and 200 km in diameter). The largest of these may lie above the boundary for hydrostatic equilibrium, but most are irregular. Most of the trans-Neptunian objects listed with a radius smaller than 200 km have "assumed sizes based on a generic albedo of 0.09" since they are too far away, with existing instruments, to directly measure their sizes. Values relative to Earth are not included beyond this point. Mass switches from 1021 kg to 1018 kg (Zg), with Mimas double listed as example of unit shift. Main-belt asteroids have orbital elements constrained by (2.0 AU < a < 3.2 AU; q > 1.666 AU) according to JPL Solar System Dynamics (JPLSSD).[32] This is not complete, missing many poorly known TNOs.[33]

Satellites of Jupiter
Satellites of Saturn
Satellites of Uranus
Satellites of Neptune
Body Image Mean radius
(km)
Mass
×1018 kg
(Zg)
Type of object Shape
Mimas
Saturn I
198.3 37.49 Satellite of Saturn regular
2003 QW90 191.5[22] 89P Kuiper belt object unknown
2002 CY248 191.5[21] KBO unknown
(145480) 2005 TB190 186.25 [34] Detached object unknown
(15789) 1993 SC 181.5[22] Trans-Neptunian objectplutino[22] unknown
(48639) 1995 TL8* 175 Kuiper belt objectbinary unknown
Nereid A
Neptune II
170 31 Satellite of Neptune irregular
148780 Altjira 9 170[22] Trans-Neptunian objectcubewano unknown
(47932) GN171 160.5[20] Trans-Neptunian objectplutino unknown
704 Interamnia M 158.31[35] 37 Main-belt asteroidF-type unknown
Hiʻiaka
Haumea I
155 20 Satellite of Haumea unknown
1995 SN55* (lost) 155 Centaur unknown
(79360) 1997 CS299 152.5[22] Kuiper belt objectbinary unknown
(79978) 1999 CC1589 152[22] Scattered-disc object unknown
(40314) 1999 KR169 152 Trans-Neptunian object unknown
52 Europa$
150.4 16.5 Main-belt asteroidC-type irregular[36]
511 Davida$ 144.7 43.8 Main-belt asteroidC-type irregular
(55636) 2002 TX300 143[37] 12 Kuiper belt objectHaumea family unknown
(47171) 1999 TC36(A1) 143[38] Kuiper belt objectTrinary (A1+A2+B) unknown
87 Sylvia$
142.8 14.78 Outer main-belt asteroidX-typetrinary irregular[36]
Vanth
Orcus I
140–190 Satellite of Orcus unknown
(26308) 1998 SM165 139.9[20] 14 Kuiper belt objectbinary unknown
65 Cybele$ 136.5[39] 2004
118.7[40] IRAS
17.8 Outer main-belt asteroidC-type irregular
Hyperion
Saturn VII
135[3] 5.58 Satellite of Saturn irregular
(47171) 1999 TC36(A2) 132.5[38] Kuiper belt objectTrinary (A1+A2+B) unknown
2005 PU219 132.5[22] Scattered-disc object unknown
(79983) 1999 DF99 132.5 Trans-Neptunian objectcubewano unknown
107 Camilla$ 129.4 11.2 Outer main-belt asteroidC-typebinary irregular[41]
10199 Chariklo 129.3 [20] Centaur unknown
31 EuphrosyneM 128 6.23 Main-belt asteroidC-type unknown
15 Eunomia$ 127.7[42] 31.2 Main-belt asteroidS-type irregular[36]
(148209) 2000 CR105*A 126.5[43] 13 Detached object unknown
(145453) 2005 RR43 126
348.4[43]
Kuiper belt objectHaumea family unknown
S/2007 (148780) 1
Altjira I
123[44] Secondary of 148780 Altjira unknown
(119878) 2002 CY224 121[22] 15 Scattered disc object unknown
3 Juno $
116.96[35] 26.7 Main-belt asteroidS-type irregular[36]
2060 Chiron*A
95P/Chiron
116.7 10 Centaur unknown
88 Thisbe $ 116[45] 10.5 M Main-belt asteroidB-type irregular[41]
(120178) 2003 OP32 115 Kuiper belt objectHaumea family unknown
2004 VN1129 115 Scattered-disc object unknown
2002 KW14 115[46] Kuiper belt object unknown
324 BambergaM 114 10 Main-belt asteroidC-type unknown
451 Patientia 112.5 Main-belt asteroid unknown
19 Fortuna $ 112.5[47] 12.7 Main-belt asteroidG-type unknown
532 Herculina 111 Main-belt asteroidS-type irregular[36]
48 Doris 110.9[48] 17A Main-belt asteroid irregular
375 Ursula
108 [49] Main-belt asteroid unknown
45 EugeniaM
File:45 eugenia-01.jpg
107 5.69 Main-belt asteroidF-typetrinary irregular[36]
Phoebe $
Saturn IX
106.6 8.29 Satellite of Saturn irregular
29 Amphitrite$ 106 11.8 Main-belt asteroidS-type irregular[36]
53311 Deucalion 105.5[22] Trans-Neptunian objectcubewano unknown
(33001) 1997 CU29 105.5 Trans-Neptunian objectcubewano unknown
423 DiotimaA 104.385[35] 16 Main-belt asteroidC-type irregular[50]
(181902) 1999 RD215 104.33[22] Scattered disc object unknown
13 EgeriaM 103.82[35] 16.3 Main-belt asteroidG-type unknown
54598 Bienor 103.5[51] Centaur unknown
94 Aurora 102.5 Main-belt asteroid irregular[52]
624 HektorA
101.5[53] 14 AsteroidJupiter Trojanbinary irregular
38083 Rhadamanthus 100.5[22] Kuiper belt object unknown
(19308) 1996 TO66 100 Kuiper belt objectHaumea family unknown

Selected objects between 100 and 50 km in radius

Objects 100 and 50 km in radius (200 km to 100 km in average diameter). This currently includes most objects in the asteroid belt and moons of the gas giants in this size range, but is missing many newly discovered objects in the outer Solar System such as here.[33] Asteroid spectral types are mostly Tholen, but some might be SMASS.

Body Image Mean radius
(km)
Mass
×1018 kg
(Zg)
Type of object
7 Iris$
99.915 [54] 13.6 Main-belt asteroidS-type
24 Themis M 99 11.3 Main-belt asteroidC-typeThemis
702 Alauda
97.4[35] 6.05 Main-belt asteroidC-typebinary
LarissaA
Neptune VII (7)
97 4.2 Satellite of Neptune
(85633) 1998 KR65 96[22] Kuiper belt objectcubewano
121 HermioneM 95 5.38 Outer main-belt asteroidC-typebinary
Actaea
Salacia I
95 Satellite of 120347 Salacia
372 Palma 94.31[55] Main-belt asteroid
128 Nemesis 94.1 7 Main-belt asteroidC-type
16 Psyche$ 93.0 21.9 Main-belt asteroidM-type
6 Hebe $ 92.59[35] 12.8 Main-belt asteroidS-type
5145 Pholus 92.5[56] 6.6 Centaur
154 Bertha 92.47[35] 5.2 Main-belt asteroidC-type
76 Freia 91.83 6.5 Outer main-belt asteroidCybele
(59358) 1999 CL1589 91.5 Trans-Neptunian object—unstable
130 ElektraM 91.1[35] 6.6 AsteroidG-typebinary
(119951) 2002 KX14 90[21] Trans-Neptunian object[21]
Janus$
Saturn X (10)
89.4 1.912 Satellite of Saturn
259 Aletheia 89.3[35] 5.97 Main-belt asteroid
Galatea
Neptune VI (6)
88[3] 2.12 Satellite of Neptune
88611 Teharonhiawako 88[22] Trans-Neptunian objectcubewanobinary
42355 Typhon 87.5[20] Trans-Neptunian objectbinary
(19255) 1994 VK8 87.5[22] 5.6 Trans-Neptunian objectcubewano
120 Lachesis 87.05[35] 5.5 Main-belt asteroid
65489 Ceto 87[57] 5.4[57] CentaurTNObinary
(24835) 1995 SM55 87 Kuiper belt objectHaumea family
41 Daphne 87 Main-belt asteroid
9 Metis$ 86.9 11.3 Main-belt asteroid
747 Winchester 85.86[35] Asteroid
153 Hilda 85.32[35] 5.2 Main-belt asteroidHildas
790 Pretoria 85.2[58] Outer main-belt asteroidCybele
Himalia M
Jupiter VI (6)
85[3]–92[59] 4.19 [60] Satellite of JupiterHimalia group
Namaka
Haumea II
85 2 Satellite of Haumea
96 Aegle 84.95 5.1 Main-belt asteroid
241 Germania 84.45[35] 5.05 Main-belt asteroidC-type
194 Prokne 84.21[35] 5 Main-belt asteroidC-type
566 Stereoskopia[61] 84.08[35] Outer main-belt asteroidCybele
Amalthea
Jupiter V (5)
83.5[62] 2.08[63] Satellite of Jupiter$
911 Agamemnon 83.3[35] AsteroidJupiter Trojan
22 Kalliope
83.1[64] 8.09M Main-belt asteroidM-typebinary
66652 Borasisi 83[22] Trans-Neptunian objectcubewanobinary
54 Alexandra 82.88 Main-belt asteroid
386 Siegena 82.5[65] Main-belt asteroidC-type
59 Elpis 82.4 Main-belt asteroid
1437 Diomedes 82.16[35] 4.6 AsteroidJupiter Trojan
444 GyptisM 81.54[35] 12.5 Main-belt asteroidC-type
Puck
Uranus XV [15]
81[3] 2.9A Satellite of Uranus
409 Aspasia 80.81[35] 4.42 Main-belt asteroidC-type
S/2002 (48639) 1 80.5 Satellite of (48639) 1995 TL8
20461 Dioretsa 80.2[22] Centaur[66]Damocloid
1992 QB1 80[22] Kuiper belt objectcubewano
(15875) 1996 TP66 80[20] Kuiper belt object— inner plutino
209 Dido 79.97[35] 4.28 Main-belt asteroidC-type
334 Chicago 79.275[35] Main-belt asteroidC-type
804 Hispania 78.79[35] 9.95 Main-belt asteroidP-type
185 Eunike 78.76[35] 4.09 Main-belt asteroid
139 Juewa 78.3[35] 4 Main-belt asteroid
354 Eleonora 77.585[35] Main-belt asteroidS-type
85 Io 77.4[67] 3.4 Main-belt asteroid
165 Loreley 77.39[35] 3.91 Main-belt asteroidC-type
173 Ino 77.05[35] 3.83 Main-belt asteroidC-type
11 Parthenope 76.67[35] 6.15M Main-belt asteroid
(137295) 1999 RB216 76.5[22] Kuiper belt objecttwotino
14 Irene 76[68] 8.2 Main-belt asteroid
89 Julia 75.75 3.6 Main-belt asteroidS-type
536 Merapi 75.7[35] Main-belt asteroid
(145474) 2005 SA278 75.62[22] Scattered-disc object
776 Berbericia 75.59[35] Main-belt asteroid
145 Adeona 75.57[35] 3.6 Main-belt asteroidAdena
150 Nuwa 75.565[35] 3.62 Main-belt asteroidC-type
Dysnomia
Eris I
75[69] Satellite of Eris
DespinaA
Neptune V
75 2.1 Satellite of Neptune
Sycorax
Uranus XVII
75[3] 2.3 Satellite of Uranus
49 Pales M 74.9[35] 2.69 Main-belt asteroidC-type
39 Laetitia 74.75 3.5 Asteroid
117 Lomia 74.36[35] 3.4 Main-belt asteroidC-type
238 Hypatia 74.245[35] Main-belt asteroidC-type
168 Sibylla 74.195[35] 3.42 Main-belt asteroidC-type
283 EmmaM 74 1.38 Asteroidbinary
51 Nemausa 73.93 Asteroid
106 Dione 73.3 Main-belt asteroidG-type
(118378) 1999 HT11 73[22] Trans-Neptunian object
137 Meliboea 72.71[35] 3.2 Main-belt asteroid
20 Massalia$ 72.5 5.67 Asteroid
211 Isolda 71.6[35] 3.07 Main-belt asteroidC-type
1172 Äneas 71.41[70] AsteroidJupiter Trojan
144 Vibilia 71.19[35] 3 Main-belt asteroid
508 Princetonia 71.18[35][71] Main-belt asteroid
895 Helio 70.95 [35] Main-belt asteroidB-type
361 Bononia 70.86 [35] Main-belt asteroidD-type
420 Bertholda 70.625 [35] Main-belt asteroidP-type
93 Minerva 70.5 2.9 Main-belt asteroidC-typetrinary
617 Patroclus 70.46 [35] AsteroidJupiter Trojanbinary
308 Polyxo 70.345[35] 2.92 Main-belt asteroidT-type
18 Melpomene 70.3 3 Main-belt asteroid
268 Adorea 69.945[35] 2.87 Main-belt asteroid
349 Dembowska 69.885[35] Main-belt asteroidR-type
489 Comacina 69.695 [35] Main-belt asteroid
(47171) 1999 TC36(B) 69.5[38] Kuiper belt objectTrinary (A1+A2+B)
69 Hesperia 69.07 2.76 Main-belt asteroidM-type
2003 UZ117 69 Kuiper belt objectHaumea family
762 Pulcova
68.54 [35] Main-belt asteroidC-typebinary
Pabu
Borasisi I
68.5[72] Secondary of 66652 Borasisi
196 Philomela 68.195[35] 2.65 Main-belt asteroidS-type
212 Medea 68.06[35] 2.64[73] Main-belt asteroid
95 Arethusa 68.02[35] 2.6 Main-belt asteroid
Portia
Uranus XII
67.6[3] 1.7 Satellite of Uranus
588 Achilles 67.735 [35] AsteroidJupiter Trojan
690 Wratislavia
67.325 [35] Asteroid
111 Ate 67.28 Main-belt asteroidC-type
247 Eukrate 67.215[35] Main-belt asteroidC-type
705 Erminia 67.11[35] Main-belt asteroid
471 Papagena 67.095 [35] Main-belt asteroidC-type
Phorcys
Ceto I
67[22] 1.67[57] Satellite of 65489 Ceto
1998 WW31 66.5 2 Trans-Neptunian objectbinary
147 Protogeneia 66.465[35] 2.5 Main-belt asteroid
Menoetius
Patroclus I
66.3 Secondary of 617 Patroclus
344 Desiderata 66.135[35] 2.42 Main-belt asteroidC-type
146 Lucina 66.1[35] 2.4 Main-belt asteroid
141 Lumen 65.52[35] 1.6 Main-belt asteroidC-type
356 Liguria 65.655 [35] Main-belt asteroid
187 Lamberta 65.2 [35] 2.37 Main-belt asteroidC-type
419 Aurelia 64.505 [35] Main-belt asteroidF-type
200 Dynamene 64.18[35] Main-belt asteroid
8 Flora 63.9 8.47 Main-belt asteroidS-typeFlora
712 Boliviana 63.785 [35] Main-belt asteroidX-type
654 Zelinda 63.7 [35] Main-belt asteroid
426 Hippo 63.55 [35] Main-belt asteroid
47 Aglaja pic 63.48 Main-belt asteroidC-type
279 Thule 63.295[35] Main-belt asteroidD-type
92 Undina 63.21[74] 2.1 Main-belt asteroidM-type
1173 Anchises(1930 UB) 63.135[35] AsteroidJupiter Trojan
1143 Odysseus 62.82[35] AsteroidJupiter Trojan (L4)
469 Argentina 62.785 [35] Main-belt asteroidCybele
159 Aemilia 62.5 1.4 Asteroid
405 Thia 62.45 [35] Main-belt asteroidC-type
602 Marianna 62.36 [35] Main-belt asteroid
46 Hestia 62.07[35] 3.5[75]–21[76] Main-belt asteroid
216 Kleopatra 62 Main-belt asteroidM-typetrinary
104 Klymene 61.9 2 Main-belt asteroid
410 Chloris 61.785 [35] Main-belt asteroidC-type
134 Sophrosyne 61.64 2 Main-belt asteroid
328 Gudrun 61.46[35] 1.94 Main-belt asteroidS-type
1867 Deiphobus 61.335[35] AsteroidJupiter Trojan
68 Leto 61.3 Main-belt asteroidS-type
70 Panopaea 61.01 Main-belt asteroidC-type
Sawiskera
Teharonhiawako I
61 Secondary of 88611 Teharonhiawako
127 Johanna 61[77] Main-belt asteroid
276 Adelheid 60.8[35] Main-belt asteroid
176 Iduna 60.52[35] 1.76 Main-belt asteroidG-type
156 Xanthippe 60.495[35] 1.85 Main-belt asteroidS-type
28 Bellona 60.45[35] Main-belt asteroidC-type
86 Semele 60.3 Main-belt asteroidC-type
78 Diana 60.3 Main-belt asteroidC-type
381 Myrrha 60.29 [35] Main-belt asteroidC-type
225 Henrietta 60.245[35] 1.83 Main-belt asteroidC-typeCybele
618 Elfriede 60.145 [35] Main-belt asteroidC-type
(73840) 2002 PN34 59.75[20] Scattered-disc object
105 Artemis 59.6 1.8 Main-belt asteroidC-type
81 Terpsichore 59.54 Main-belt asteroidC-type
5 Astraea 59.535[35] 2.9 Main-belt asteroid
74 Galatea 59.36 1.8 Main-belt asteroidC-type
350 Ornamenta 59.175[35] Main-belt asteroidC-type
772 Tanete 58.83[35] Main-belt asteroidC-type
476 Hedwig 58.38 [35] Main-belt asteroid
1093 Freda 58.365 [35] Main-belt asteroid
171 Ophelia 58.35[35] 1.66 Main-belt asteroidC-typeThemis
909 Ulla 58.22[35] Asteroid
3317 Paris 58.13[35] AsteroidJupiter Trojan
203 Pompeja 58.125[35] Main-belt asteroid
3063 Makhaon 58.07[35] 1.6 AsteroidJupiter Trojan
38 Leda 57.97[35] 1.6 Asteroid
360 Carlova 57.88[35] Main-belt asteroid
521 Brixia 57.825 [35] Main-belt asteroid
490 Veritas 57.775[35] Main-belt asteroid—Veritas
466 Tisiphone 57.765 [35] Main-belt asteroidC-type
53 Kalypso 57.69 Asteroid
2241 Alcathous 57.315 [35] AsteroidJupiter Trojan
388 Charybdis 57.085 [35] Main-belt asteroidC-type
34 Circe 56.75 1.5 Main-belt asteroidC-type
Epimetheus
Saturn XI (11)
56.7[3] 0.5304[78] Satellite of Saturn$
596 Scheila 56.67 [35] Main-belt asteroid
56 Melete 56.62 1.5 Asteroid
129 Antigone 56.5[79] 2 Main-belt asteroid—nickel-iron
12 Victoria 56.4 Main-belt asteroidS-type
57 Mnemosyne 56.3 Asteroid
545 Messalina 55.645 [35] Asteroid
2797 Teucer 55.57[35] AsteroidJupiter Trojan(L4)
2920 Automedon 55.5[35] AsteroidJupiter Trojan(L4)
2001 QR322 55 Neptune trojan
91 Aegina 54.9 1.4 Main-belt asteroidC-type
140 Siwa 54.895 [35] 1.4 Main-belt asteroid
814 Tauris 54.78[35] Main-belt asteroid
595 Polyxena 54.535 [35] Main-belt asteroid
230 Athamantis 54.495 Main-belt asteroidS-type
659 Nestor 54.435 [35] AsteroidJupiter Trojan
37 Fides 54 1.3 Main-belt asteroidS-type
514 Armida 53.085 [35] Main-belt asteroid
23 Thalia 53.8 1.3 Main-belt asteroidS-type
739 Mandeville 53.765 [35] Main-belt asteroidX-type
2007 VL305 A 53.75 Neptune trojan
40 Harmonia 53.6 1.3 Main-belt asteroidS-type
181 Eucharis 53.33[35] 1.2 Main-belt asteroidK-type
346 Hermentaria 53.26 [35] Main-belt asteroidS-type
357 Ninina 53.05 [35] Main-belt asteroid
506 Marion 52.97 [35] Main-belt asteroidC-type
365 Corduba 52.96 [35] Main-belt asteroidC-type
36 Atalante 52.8 Asteroid
713 Luscinia 52.76 [35] Main-belt asteroidC-type
1269 Rollandia 52.595[35] Main-belt asteroid
164 Eva 52.435[35] 1.21 Main-belt asteroidC-type
98 Ianthe 52.25 1.2 Main-belt asteroidC-type
240 Vanadis 51.95 [35] Main-belt asteroidC-type
221 Eos 51.935[35] 1.17 Main-belt asteroidK-type
(29981) 1999 TD10 51.85[20] Trans-Neptunian object
788 Hohensteina 51.84[35] Main-belt asteroid
791 Ani 51.76[35] Main-belt asteroid
1208 Troilus 51.67[35] AsteroidJupiter Trojan
192 Nausikaa 51.63[35] Main-belt asteroidS-type
63 Ausonia 51.57 1.1 Main-belt asteroidS-type
35 Leukothea 51.555[35] 1.1 Main-belt asteroidC-type
570 Kythera 51.405 [35] Main belt asteroid
233 Asterope 51.39 [35] 1.4 Main belt asteroidT-type
4063 Euforbo 51.23[35] AsteroidJupiter Trojan
1583 Antilochus 50.81[35] AsteroidJupiter Trojan
1390 Abastumani 50.79[35] Main-belt asteroid
522 Helga 50.61 [35] Main-belt asteroidCybele
175 Andromache 50.585[35] 1.08 Main-belt asteroidC-type
191 Kolga 50.515[35] 1.08 Main-belt asteroidC-type
663 Gerlinde 50.44 [35] Asteroid
626 Notburga 50.365 [35] Asteroid
387 Aquitania 50.255[35] Main-belt asteroidS-type
42 Isis 50.1 Main-belt asteroidS-type
30 Urania 50 Main-belt asteroidS-type

Examples of objects between 50 km and 20 km in radius

There are easily tens of thousands of objects 50 km in radius or smaller[clarification needed], but only a fraction have been explored. The number of digits is not an endorsement of significant figures. The table switches from ×1018 kg to ×1015 kg (Eg), and many of these mass values are assumed. (see also List of minor planets)

Body Image Mean radius
(km)
Mass
×1015 kg
(Eg)
Type of object
50 VirginiaA 49.91 1000 Asteroid
114 Kassandra 49.86[35] 1000 Main-belt asteroidT-type
1021 Flammario 49.695[35] Asteroid
162 Laurentia 49.55[35] Main-belt asteroid
401 Ottilia 49.56[35] Main-belt asteroid
ThebeA
Jupiter XIV (14)
49.3[3] 430 Satellite of Jupiter
148 Gallia 48.88[35] 980 Main-belt asteroidR-type
404 Arsinoe 48.855[35] Main-belt asteroidC-type
27 EuterpeA 48 930 Main-belt asteroidS-type
773 Irmintraud 47.94[35] AsteroidD-type
21 Lutetia
File:21 Lutetia.jpg
47.8[35] 1700 [80] Main-belt asteroidM-type
62 Erato 47.7 910 Main-belt asteroidThemis
26 Proserpina 47.4[35] 900 Asteroid
345 Tercidina 47.06[35] Main-belt asteroidC-type
JulietA
Uranus XI
46.8[3] 560 Satellite of Uranus
58 Concordia 46.72 850 Asteroid
229 Adelinda 46.6[35] Main-belt asteroidC-type
379 Huenna 46.2 480 Main-belt asteroidC-type
Nix
Pluto II
46[81] 70 Satellite of Pluto
103 Hera 45.6 790 Asteroid
17 Thetis
45 1200 Asteroid
143 Adria 44.965[35] 760 Main-belt asteroid
109 Felicitas 44.7 750 Asteroid
100 Hekate 44.5[82] 1000 Asteroid
90 Antiope A
File:90 Antiope.gif
43.9[83] 410 AsteroidC-typebinary
227 Philosophia 43.655[35] Main-belt asteroid
Prometheus $
Saturn XVI (16)
43.1[84] 156.6 Satellite of Saturn
110 Lydia 43.05 670 Asteroid
ElaraA
Jupiter VII
43 870 Satellite of JupiterHimalia group
72 Feronia 42.95 670 Asteroid
60558 Echeclus/
174P/Echeclus
42[20][22] Centaur[85]
S/2000 (90) 1
File:90 Antiope.gif
41.9[83] Asteroid moon of 90 Antiope
71 Niobe 41.7 610 Asteroid
102 Miriam 41.5[86] Asteroid
97 Klotho 41.4 590 Asteroid
61 Danae 41.02 Asteroid
ThalassaA
Neptune IV
41 350 Satellite of Neptune
122 Gerda 40.85[35] 570 Main-belt asteroidS-type
Pandora$
Saturn XVII (17)
40.7[84] 135.6 Satellite of Saturn
83 Beatrix 40.69 560 Main-belt asteroidX-type
32 PomonaA 40.5 550 Asteroid
BelindaA
Uranus XIV (14)
40 360 Satellite of Uranus
115 Thyra 39.92[35] Asteroid
Cressida
Uranus IX
39.8[3] 340A Satellite of Uranus
135 Hertha 39.62[35] Asteroid
84 Klio 39.58[87] 520 Asteroid
80 Sappho 39.2 Asteroid
Echidna
Typhon I
39 Satellite of 42355 Typhon
1001 Gaussia 39 Asteroid
58534 Logos 38.5[88] 270 Kuiper belt objectcubewanobinary
124 Alkeste 38.18[35] 470 Main-belt asteroidS-type
55576 Amycus 38.15[20] Centaur
25 Phocaea 37.6 Asteroid
Weywot
Quaoar I
37 Satellite of Quaoar
8405 Asbolus 37[89]–42[20] Centaur
112 Iphigenia 36.35[35] Asteroid
(86047) 1999 OY3 36 Kuiper belt objectHaumea family
Hydra
Pluto III
36[3] 391P Satellite of Pluto
Rosalind*
Uranus XIII
36 250 Satellite of Uranus
Caliban
Uranus XVI
36[3] Satellite of Uranus
99 Dike 35.95 390 Asteroid
66 Maja 35.91 Asteroid
116 Sirona 35.85[35] Main-belt asteroid
44 Nysa 35.32 370 Main-belt asteroidE-type
10370 Hylonome 35[20] Centaur
77 Frigga 34.63 350 Asteroid
55 Pandora 33.35 Asteroid
133 Cyrene 33.29[35] 310 Main-belt asteroidS-type
79 Eurynome 33.24 Asteroid
Zoe
Logos I
33 Satellite of 58534 Logos
Naiad
Neptune III
33 190A Satellite of Neptune
43 Ariadne 32.94[35] Asteroid
101 Helena 32.9 300 Asteroid
108 Hecuba 32.49[90] 390 Asteroid
DesdemonaA
Uranus X
32 180 Satellite of Uranus
Halimede*
Neptune IX
31 Satellite of Neptune
52975 Cyllarus 31[20] Centaur
82 Alkmene 30.48 Asteroid
60 Echo 30.1 Asteroid
Crantor
83982
30[91] Centaur
Comet Hale–Bopp
C/1995 O1
30[92] Comet
Pasiphaë*A
Jupiter VIII
30 300 Satellite of Jupiter
7066 Nessus 30[20][22] Centaur
Neso
Neptune XIII
30[3] Satellite of Neptune
64 Angelina 30[93] Main-belt asteroidE-type
2008 KV42 29.5[94] Detached object
67 Asia 29.06 Asteroid
119 Althaea 28.65[35] 200 Main-belt asteroidS-type
75 Eurydike 27.955[35] 180 Main-belt asteroidM-type
142 Polana 27.645[35] 180 Main-belt asteroidF-type
253 Mathilde$
26.4 103.3 Main-belt asteroidC-type
52872 Okyrhoe 26.01[20] Centaur
Bianca
Uranus VIII
25.7[3] 92 Satellite of Uranus
Prospero
Uranus XVIII
25 85 Satellite of Uranus
Setebos
Uranus XIX
24[3] 75 Satellite of Uranus
123 Brunhild 23.985[35] Main-belt asteroid
4348 Poulydamas 23.95[95] AsteroidJupiter Trojan
1000 Piazzia 23.89[35] Main-belt asteroid
113 Amalthea 23.07[35] 100 Main-belt asteroid
Carme*
Jupiter IX
23 130 Satellite of JupiterCarme group
138 Tolosa 22.75[35] 99 Main-belt asteroidS-type
126 Velleda 22.4[35] 94 Main-belt asteroid
73 Klytia 22.22 92 Asteroid
Sao
Neptune XI
22 Satellite of Neptune
125 Liberatrix 21.79[35] 87 Main-belt asteroidM-type
Metis
Jupiter XVI (16)
21.5[96] 36 Satellite of Jupiter
132 Aethra 21.435[35] 82 Main-belt asteroidM-type
Ophelia*
Uranus VII
21.4[3][4] 53 Satellite of Uranus
Laomedeia
Neptune XII
21 Satellite of Neptune
118 Peitho 20.87[35] 76 Main-belt asteroid
208 Lacrimosa 20.665[35] 73.9 Main-belt asteroidKoronisS-type
136 Austria 20.5[35] 68 Main-belt asteroidM-type
131 Vala 20.22[35] 69 Main-belt asteroid
Cordelia*
Uranus VI
20.1[3] 44 Satellite of Uranus
Siarnaq
Saturn XXIX
20[84] Satellite of Saturn

Examples of objects between 20 km and 1 km in radius

Satellites of Jupiter
Satellites of Saturn
Satellites of Uranus
Satellites of Neptune
Body Image Mean
radius
(km)
Mass
×1015 kg
(Eg)
Type of object
167 Urda 19.97[35] 66.7 Main-belt asteroidKoronisS-type
Hidalgo
944
19 Centaur
Sinope*
Jupiter IX
19 76 Satellite of Jupiter
Psamathe*
Neptune X
19 37 Satellite of Neptune
29P/Schwassmann–
Wachmann
18.65[20] Cometcentaur
Lysithea*
Jupiter X
18 63 Satellite of JupiterHimalia group
158 Koronis 17.685[35] 46.3 Main-belt asteroidKoronisS-type
Helene
Saturn XII (12)
Dione B
17.6[3] 25 Satellite of SaturnDione trojan
226 Weringia 16.92[35] Main-belt asteroidS-type
433 Eros$
16.84 66.9 Near-Earth asteroidAmor
Stephano
Uranus XX
16[3] 22 Satellite of Uranus
Albiorix
Saturn XXVI (16)
16 Satellite of Saturn
1036 Ganymed 15.9 33 Near-Earth asteroid
1815 Beethoven 15.8[22] Main-belt asteroid
243 Ida
15.7[97] 42 Main-belt asteroidKoronisS-typebinary
Atlas$
Saturn XV (15)
15.3 66 Satellite of Saturn
31824 Elatus 15[20] Centaur
Perdita
Uranus XXV (15)
15[98] 13 Satellite of Uranus
Pan$
Saturn XVIII (18)
14.2[99] 4.95[99] Satellite of Saturn
Linus
Kalliope I
14[64] 60[100] Asteroid moon of 22 Kalliope
Ananke
Jupiter XII (12)
14[59] 38.2 Satellite of Jupiter
Telesto
Saturn XIII or Tethys B
11.8[101] Satellite of SaturnTethys trojan
Phobos$
Mars I
11.1 10.7 Satellite of Mars
Paaliaq
Saturn XX - 20
11 8.2 Satellite of Saturn
Francisco
Uranus XXII - 22
11[3] 7.2 Satellite of Uranus
Calypso
Saturn XIV or Tethys C
10.7[3] Satellite of SaturnTethys trojan
Leda
Jupiter XIII (13)
10[3] 11 Satellite of JupiterHimalia group
Ferdinand
Uranus XXIV - 24
10[3] 5.4 Satellite of Uranus
Margaret
Uranus XXIII - 23
10[3] 5.4 Satellite of Uranus
149 Medusa 9.88[35] 8 Main-belt asteroid
Romulus
Sylvia I
9 4 Asteroid moon of 87 Sylvia
Ymir
Saturn XIX (19)
9[3] Satellite of Saturn
Trinculo
Uranus XXI - 21
9 3.9 Satellite of Uranus
Cupid
Uranus XXVII - 27
9 3.8 Satellite of Uranus
2002 Euler 8.72 5.5 Asteroid
Adrastea
Jupiter XV (15)
8.2[3] 2 Satellite of Jupiter
Kiviuq
Saturn XXIV - 24
8[3] Satellite of Saturn
2000 Herschel 8[102] Main-belt asteroid[103]
Tarvos
Saturn XXI (21)
7.5[3] Satellite of Saturn
S/2006 (624) 1
Hektor I
7.5 Asteroid moon of 624 Hektor
2685 Masursky
7–10 5–11 Asteroid
(65407) 2002 RP120 7.3[104] 3.1 Damocloid (retrograde) & possible ejected SDO
Bestla
Saturn XXXIX - 34
7 Satellite of Saturn
S/2011 P 1
Pluto IV
6.5–17 Satellite of Pluto
Petit-Prince
Eugenia I
6.5 1.2 Asteroid moon of 45 Eugenia
Deimos$
Mars II
6.2 1.48 Satellite of Mars
951 Gaspra
6.1[105] 2–3 Asteroid
Ijiraq
Saturn XXII - 22
6 Satellite of Saturn
S/2002 (121) 1
Hermione I
6[106] 1.6 Asteroid moon of 121 Hermione
1P/Halley
5.5[107] 0.03[108] Comet (75.3 year period)
S/2001 (107) 1
Camilla I
5.5[106] 1.5 Asteroid moon of 107 Camilla
Mab
Uranus XXVI (26)
5.0[109] Satellite of Uranus
Erriapus
Saturn XXVIII - 18
5.0 Satellite of Saturn
26858 Misterrogers 4.75 Asteroid
Callirrhoe
Jupiter XVII - 17
4.3 Satellite of Jupiter
Themisto
Jupiter XVIII - 38
4.0 0.69 Satellite of Jupiter
Daphnis
Saturn XXXV (35)
3.9 [110] 0.084[99] Satellite of Saturn
Remus
Sylvia II
3.5 0.2 Asteroid moon of 87 Sylvia
S/2003 (379) 1
Huenna I
3.5 Asteroid moon of 379 Huenna
Tarqeq
Saturn LII - 52
3.5 Satellite of Saturn
Kari
Saturn XLV - 45
3.5 Satellite of Saturn
Mundilfari
Saturn XXV - 25
3.5 Satellite of Saturn
Suttungr
Saturn XXIII - 23
3.5 Satellite of Saturn
Praxidike
Jupiter XXVII - 27
3.4 Satellite of Jupiter
Narvi
Saturn XXXI - 31
3.3 Satellite of Saturn
Skathi
Saturn XXVII - 27
3.2 Satellite of Saturn
9P/Tempel
3[111][112] 0.075 Comet
Hyrrokkin
Saturn XLIV - 44
3.0[3] Satellite of Saturn
Greip
Saturn LI - 51
3 Satellite of Saturn
Jarnsaxa
Saturn L - 50
3 Satellite of Saturn
Skoll
Saturn XLVII - 47
3 Satellite of Saturn
Surtur
Saturn XLVIII - 48
3 Satellite of Saturn
S/2003 (130) 1
Elektra I
3 0.4 Asteroid moon of 130 Elektra
Loge
Saturn XLVI - 46
3 Satellite of Saturn
Hati
Saturn XLIII - 43
3 Satellite of Saturn
Fornjot
Saturn XLII - 42
3 Satellite of Saturn
Bebhionn
Saturn XXXVII - 37
3 Satellite of Saturn
Aegir
Saturn XXXVI - 36
3 Satellite of Saturn
S/2004 (45) 1
Eugenia II
3 Asteroid moon of 45 Eugenia
S/2007 S 2 3 Satellite of Saturn
118401 LINEAR 3 0.23 Main-belt comet
Bergelmir
Saturn XXXVIII (38)
3[3] Satellite of Saturn
Thrymr
Saturn XXX (30)
2.8[113] Satellite of Saturn
4179 Toutatis
2.7[114] 0.05 Near-Earth asteroid
Megaclite
Jupiter XIX (19)
2.7[3]
–2.25[115]
Satellite of Jupiter
2867 Šteins 2.65[116] AsteroidE-type
Iocaste
Jupiter XXIV - 24
2.6 Satellite of Jupiter
Kalyke
Jupiter XXIII - 23
2.6 Satellite of JupiterCarme group
3200 Phaethon 2.55 14 AsteroidApolloB-type
Farbauti
Saturn XL - 40
2.5 Satellite of Saturn
3753 Cruithne 2.5 .13 Asteroid & quasi-satellite of Earth
5535 Annefrank
2.4 Asteroid
19P/Borrelly
2.4[117] Comet (6.85 year period) (Jupiter family)
2P/Encke
2.4[118] Comet (3.3 year period)
Taygete
Jupiter XX - 20
2.2 Satellite of JupiterCarme group
Harpalyke
Jupiter XXII - 22
2.2 Satellite of Jupiter
C/1996 B2
Comet Hyakutake
2.1[119] Comet[120]
81P/Wild
Wild 2
2[121] Comet
Fenrir
Saturn XLI - 41
2 Satellite of Saturn
Pallene
Saturn XXXIII (33)
2 0.043 Satellite of Saturn
Eukelade
Jupiter XLVII - 47
2 Satellite of Jupiter
Helike
Jupiter XLV - 65
2 Satellite of Jupiter
Aoede
Jupiter XLI - 41
2 Satellite of Jupiter
Hermippe
Jupiter XXX - 30
2 Satellite of Jupiter
Thyone
Jupiter XXIX - 29
2 Satellite of Jupiter
Autonoe
Jupiter XXVIII - 28
2 Satellite of Jupiter
Isonoe
Jupiter XXVI - 26
1.9 Satellite of JupiterCarme group
Chaldene
Jupiter XXI - 21
1.9 Satellite of JupiterCarme group
(53319) 1999 JM8
1.75 Asteroid
Polydeuces
Saturn XXXIV (34)
Dione C
1.75[122] 0.03 Satellite of SaturnDione trojan
17P/Holmes
1.7[123] Comet
Erinome
Jupiter XXV - 25
1.6 Satellite of JupiterCarme group
Methone
Saturn XXXII (32)
1.6[3] 0.019 Satellite of Saturn
Arche
Jupiter XLIII - 63
1.5 Satellite of Jupiter
Hegemone
Jupiter XXXIX - 34
1.5 Satellite of Jupiter
Euanthe
Jupiter XXXIII - 33
1.5 Satellite of Jupiter
Eurydome
Jupiter XXXII - 32
1.5 Satellite of Jupiter
Carpo
Jupiter XLVI - 66
1.5 0.45 Satellite of Jupiter
Aitne
Jupiter XXXI - 31
1.5 Satellite of Jupiter
4055 Magellan
File:30June2010-4055Magellan.png
1.245[124] AsteroidAmorV-type
9969 Braille
1.28 Asteroid
132524 APL
1.15 Asteroid
(6178) 1986 DA 1.15[125] 0.002 AsteroidAmorM-type
Anthe
Saturn XLIX - 49
1 Satellite of Saturn
Kore
Jupiter XLIX (49)
1 Satellite of Jupiter
Cyllene
Jupiter XLVIII (48)
1 Satellite of Jupiter
Kallichore
Jupiter XLIV (44)[126]
1 Satellite of Jupiter
Mneme
Jupiter XL (40)
1 Satellite of Jupiter
Pasithee
Jupiter XXXVIII (38)
1 Satellite of Jupiter
Kale
Jupiter XXXVII (37)
1 .015 Satellite of Jupiter
Sponde
Jupiter XXXVI (36)
1 Satellite of Jupiter
Orthosie
Jupiter XXXV (35)
1 Satellite of Jupiter
Herse
Jupiter L (50)
1 Satellite of Jupiter
Thelxinoe
Jupiter XLII (42)[126]
1 Satellite of Jupiter
Euporie
Jupiter XXXIV (34)
1[3] 0.015 Satellite of Jupiter

Examples of objects below 1 km (1000 m) in radius

In the asteroid belt alone there are estimated to be between 1.1 and 1.9 million objects with a radius above 0.5 km,[127] many of which are in the range 0.5–1.0 km. Countless more have a radius below 0.5 km.

Very few objects in this size range have been explored or even imaged. The exceptions are objects that have been visited by a probe, or have passed close enough to Earth to be viewed by large telescopes. Radius is by mean geometric radius. Number of digits not an endorsement of significant figures. Mass scale shifts from × 1015 to 1012 kg, which is 1015 grams (Petagram - Pg).

Body Image Mean
radius
meters
Mass
×1012 kg
Type of object
1620 Geographos
885[35] 4 Near-Earth asteroidApollo
1862 Apollo 850 5.1 Near-Earth asteroidApolloQ-type
100000 Astronautica ≈800[128] Inner Main-belt Asteroid[129]
Dactyl
Ida I
700 Asteroid moon of 243 Ida
1566 Icarus 700 2.9 Near-Earth asteroidApolloU-type
4769 Castalia 700[130] 1.3[131] Near-Earth asteroidApollo
(137108) 1999 AN10 650 Near-Earth asteroidApollo
(29075) 1950 DA
600 3[132] Near-Earth asteroidApollo
(66391) 1999 KW4
600 2.33 Mercury-crosser asteroidAten
46P/Wirtanen 600 Comet
103P/Hartley
Hartley 2
570

[133]

0.3[133] Comet (6.46-year period)
3908 Nyx 520 5 Near-Earth asteroidAmorV-type
S/2003 J 9 500[3] Satellite of JupiterCarme group
S/2003 J 12 500[3] Satellite of Jupiter
14827 Hypnos 450[134] Comet (dormant)[135]
2007 CA19 432 1.2 Near-Earth asteroidApollo
2062 Aten 450 0.76[136] Near-Earth asteroidAten
6489 Golevka 350[137] Near-Earth asteroidApollo
25143 Itokawa 346 0.0358 Near-Earth asteroidApollo
2004 XP14 300 Near-Earth asteroidApollo
(144898) 2004 VD17 290 3[138] Near-Earth asteroidApollo
Aegaeon
Saturn LIII
250 Satellite of Saturn
4660 Nereus
165[139] Near-Earth asteroidApollo
2005 YU55 [140]
155-170[141] Near-Earth asteroidApolloPHO[142]
S/2009 S 1
Saturn LXII (62)
150 Satellite of Saturn
2010 TK7 150 Earth trojanApollo
99942 Apophis 135 0.05[138] Near-Earth asteroidAtenPHO
2007 TU24
125[143] Near-Earth asteroidApolloPHO
2002 JE9 100 NEAApolloPHO
2010 XC15 100 NEAApolloPHO
1994 WR12 65[144] 0.002[138] Near-Earth asteroidAten
2008 HJ [ 18 [145] 0.000005 [145] Near-Earth asteroid & fast rotator (42 s)[145]
1998 KY26 15[146] Near-Earth asteroid & fast rotator (10 m)

Currently most of the objects of mass between 109 kg to 1012 kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids. (See also: list of NEAs by distance from Sun.) Note that 1994 WR12 possesses less mass than the Great Pyramid of Giza, 5.9 × 109 kg.

For more about really small objects in the Solar System see meteoroid, micrometeoroid, and interplanetary dust cloud.

Surface gravity

The surface gravity at the equator of a body can in most cases be accurately calculated using Newton's law of universal gravitation and centrifugal force.

The gravitational acceleration at the equator is given by Newton's law of universal gravitation. The formula that follows from this law is:

where

ag is the magnitude of the gravitational acceleration
G is the gravitational constant
m is the mass of the celestial body
r is the equatorial radius of the celestial body (if this varies significantly, the mean equatorial radius is used)

The magnitude of the outward acceleration due to centrifugal force is given by

where

T is the rotation period of the celestial body

The surface gravity at the equator is then given by

Closely imaged objects

Selected closely imaged objects (ordered by size; not to scale)
File:TheSun.png
Sun Jupiter Saturn Uranus Neptune Earth Venus
Mars Ganymede Titan Mercury Callisto Io Moon
Europa Triton Titania Rhea Oberon Iapetus Umbriel
File:Ariel-NASA.jpg
Ariel Dione Tethys Vesta Enceladus Miranda Proteus
File:21 Lutetia.jpg
Mimas Hyperion Phoebe Janus Amalthea Epimetheus Lutetia
Prometheus Pandora Mathilde Helene Ida Atlas Telesto
Phobos Deimos Gaspra Tempel 1 Borrelly Wild 2 Hartley 2

Notes

Using equatorial radius and assuming body is spherical
Using three radii and assuming body is spheroid
* Radius is known only very approximately
R Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft
9 Unknown radius, generic assumed albedo of 0.09
$ Well studied asteroid or moon where the dimensions and mass are very well known. Asteroid sizes and masses taken from James Baer's (Bio) personal website.
M Mass has been determined by perturbation. For asteroids, see James Baer's personal website.
A Assumed mass
P Mass calculated assuming Pluto's density of 2.0 g/cm3
Note: For many of the well-determined moons, radii were taken from the JPL Solar System Dynamics page.
O Radius has been determined with Asteroid occultation

References

  1. ^ Mike Brown. "The Dwarf Planets". CalTech. Archived from the original on 2011-02-12. Retrieved 2008-09-25. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  2. ^ D. T. Britt; G. J. Consol-magno SJ; W. J. Merline (2006). "Small Body Density and Porosity: New Data, New Insights" (PDF). Lunar and Planetary Science XXXVII. Retrieved 2008-12-16.{{cite web}}: CS1 maint: multiple names: authors list (link)
  3. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 2008-10-24. Retrieved 2008-12-16. Cite error: The named reference "jplssd" was defined multiple times with different content (see the help page).
  4. ^ a b Williams, Dr. David R. (2007-11-23). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). Archived from the original on 2010-01-18. Retrieved 2008-12-12. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  5. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae Mike Brown, How many dwarf planets are there in the outer solar system?[1]
  6. ^ Densities of those KBOs whose masses are uncertain are assumed to be 2.0 in line with Pluto
  7. ^ Jacobson, R. A. (2006). "The gravity field of the saturnian system from satellite observations and spacecraft tracking data". The Astronomical Journal. 132 (6): 2520–2526. Bibcode:2006AJ....132.2520J. doi:10.1086/508812. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |month= ignored (help)
  8. ^ "Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation" (PDF). European Planetary Science Congress Abstracts. 6. 2011. Retrieved 2011-09-14.
  9. ^ M.E. Brown and E.L. Schaller (2007). "The Mass of Dwarf Planet Eris". Science. 316 (5831): 1585. Bibcode:2007Sci...316.1585B. doi:10.1126/science.1139415. PMID 17569855. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  10. ^ Young, Eliot F.; Young, L. A.; Buie, M. (2007). "Pluto's Radius". American Astronomical Society, DPS meeting #39, #62.05; Bulletin of the American Astronomical Society. 39: 541. Bibcode:2007DPS....39.6205Y.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  11. ^ Space Daily - SATURN DAILY DLR Researchers Compile Atlas Of Saturn's Moon Rhea, An Icy Alien World (2010)
  12. ^ Thomas, P. C. (2007). "Shapes of the Cronian icy satellites and their significance". Icarus. 190 (2): 573–584. Bibcode:2007Icar..190..573T. doi:10.1016/j.icarus.2007.03.012. {{cite journal}}: Cite has empty unknown parameter: |month= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help) [dead link]
  13. ^ a b T.L. Lim, J. Stansberry, T.G. Müller (2010). ""TNOs are Cool": A survey of the trans-Neptunian region III. Thermophysical properties of 90482 Orcus and 136472 Makemake". Astronomy and Astrophysics. 518: L148. Bibcode:2010A&A...518L.148L. doi:10.1051/0004-6361/201014701.{{cite journal}}: CS1 maint: multiple names: authors list (link) Cite error: The named reference "Lim2010" was defined multiple times with different content (see the help page).
  14. ^ B. Sicardy; et al. (2006). "Charon's size and an upper limit on its atmosphere from a stellar occultation". Nature. 439 (7072): 52. Bibcode:2006Natur.439...52S. doi:10.1038/nature04351. PMID 16397493. {{cite journal}}: Explicit use of et al. in: |author= (help)
  15. ^ Michael E. Brown. "The largest Kuiper belt objects". In M. Antonietta Barucci, Hermann Boehnhardt, Dale P. Cruikshank (ed.). The Solar System Beyond Neptune (pdf). University of Arizona Press. pp. 335–345. ISBN 0-8165-2755-5.{{cite book}}: CS1 maint: multiple names: editors list (link)
  16. ^ Michael E. Brown; Burgasser, A.J.; Fraser W.C. (2011). "The Surface Composition of Large Kuiper Belt Object 2007 OR10" (PDF). Mike Brown's Website. arXiv:1108.1418. Retrieved 2011-08-08.{{cite web}}: CS1 maint: multiple names: authors list (link)
  17. ^ J. Stansberry, W. Grundy, M. Brown; et al. (2008). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". The Solar System beyond Neptune. University of Arizona Press. arXiv:astro-ph/0702538. Bibcode:2008ssbn.book..161S. {{cite journal}}: Explicit use of et al. in: |author= (help)CS1 maint: multiple names: authors list (link)
  18. ^ a b Pedro Lacerda and David C. Jewitt - Densities of Solar System Objects from their Rotational Lightcurves (2006)- Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822
  19. ^ a b c Brown, Michael E. (2010). "Quaoar: A Rock in the Kuiper belt". The Astrophysical Journal. 714 (2): 1547. arXiv:1003.5911. Bibcode:2010ApJ...714.1547F. doi:10.1088/0004-637X/714/2/1547. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help) Cite error: The named reference "Brown2010" was defined multiple times with different content (see the help page).
  20. ^ a b c d e f g h i j k l m n o p q r s John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". University of Arizona, Lowell Observatory, California Institute of Technology, NASA Ames Research Center, Southwest Research Institute, Cornell University. arXiv:astro-ph/0702538. Bibcode:2008ssbn.book..161S.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  21. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae Wm. Robert Johnston (7 August 2010). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 2011-03-03.
  22. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z Wm. Robert Johnston (22 August 2008). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 2008-12-08. Cite error: The named reference "johnston" was defined multiple times with different content (see the help page).
  23. ^ Marc W. Buie (2010-06-16 using 19 of 19 observations over 0.98 years (356 days)). "Orbit Fit and Astrometric record for 10KZ39". SwRI (Space Science Department). Retrieved 2011-08-18. {{cite web}}: Check date values in: |date= (help)
  24. ^ "2010 KZ39". IAU Minor Planet Center. Retrieved 2011-08-18.
  25. ^ Densities of those KBOs whose masses are uncertain are assumed to be 2.0 in line with Pluto
  26. ^ a b Wm. Robert Johnston (7 August 2010). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 2011-04-09.
  27. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  28. ^ Schmidt, B. E.; et al. (2008). "Hubble takes a look at Pallas: Shape, size, and surface" (PDF). 39th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXIX). Held March 10–14, 2008, in League City, Texas. 1391: 2502. Retrieved 2008-08-24. {{cite journal}}: Explicit use of et al. in: |author= (help)
  29. ^ Baer, James (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" (PDF). Celestial Mechanics and Dynamical Astronomy. 100 (2008). Springer Science+Business Media B.V. 2007: 27–42. Bibcode:2008CeMDA.100...27B. doi:10.1007/s10569-007-9103-8. Retrieved 2008-11-11. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  30. ^ "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 2006-07-13. Archived from the original on 2010-01-18. Retrieved 2008-02-09. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  31. ^ Wm. Robert Johnston (26 November 2008). "(119979) 2002 WC19". Johnston's Archive. Retrieved 2009-03-04.
  32. ^ "JPL definition of Main-belt Asteroid (MBA)". JPL Solar System Dynamics. Retrieved 2009-03-12.
  33. ^ a b "List of known trans-Neptunian objects". Johnstonsarchive.net. 2010-08-07. Archived from the original on 2007-06-20. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  34. ^ Muller, T.G. (2010). ""TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)". Astronomy and Astrophysics. 518: L146. Bibcode:2010A&A...518L.146M. doi:10.1051/0004-6361/201014683. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  35. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz da db dc dd de df dg dh di dj dk dl dm dn do dp dq dr ds dt du dv dw dx dy dz ea eb ec ed ee ef eg eh ei ej ek el em en eo ep eq er es et eu ev ew ex ey ez fa fb fc fd fe ff fg fh fi fj fk fl fm fn fo fp fq fr fs ft fu fv Asteroid Data Archive, Archive Planetary Science Institute
  36. ^ a b c d e f g M. Kaasalainen (2002). "Models of Twenty Asteroids from Photometric Data" (PDF). Icarus. 159 (2): 369. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907. Retrieved 2009-06-23.
  37. ^ Clara Moskowitz (2010-06-16). "Scientists size up a bright mini-world". MSNBC. Retrieved 2010-06-16.
  38. ^ a b c Benecchi, S.D (2010). "(47171) 1999 TC36, A Transneptunian Triple". Icarus. 207 (2): 978–991. arXiv:0912.2074. Bibcode:2010Icar..207..978B. doi:10.1016/j.icarus.2009.12.017. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  39. ^ Müller, T. G (2004). "65 Cybele in the thermal infrared: Multiple observations and thermophysical analysis". Astronomy and Astrophysics. 418 (1): 347–356. arXiv:astro-ph/0401458. Bibcode:2004A&A...418..347M. doi:10.1051/0004-6361:20040025. {{cite journal}}: |access-date= requires |url= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  40. ^ "JPL Small-Body Database Browser: 65 Cybele". 2008-08-10 last obs. Archived from the original on 2010-01-17. Retrieved 2008-11-25. {{cite web}}: Check date values in: |date= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  41. ^ a b J. Torppa; et al. (2003). "Shapes and rotational properties of thirty asteroids from photometric data" (PDF). Icarus. 164 (2): 346. Bibcode:2003Icar..164..346T. doi:10.1016/S0019-1035(03)00146-5. {{cite journal}}: Unknown parameter |author-separator= ignored (help)
  42. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  43. ^ a b "List of Known Trans-Neptunian Objects". Johnston's Archive. Archived from the original on 2007-06-20. Retrieved 2006-12-14. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  44. ^ Johnston's Archive about (148780) Altjira
  45. ^ "JPL Small-Body Database Browser: 88 Thisbe". 2008-07-04 last obs. Retrieved 2008-11-06. {{cite web}}: Check date values in: |date= (help)
  46. ^ "2002 KW14". Sphinx.planetwaves.net. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  47. ^ Storrs, Alex (1998). "Imaging Observations of Asteroids with Hubble Space Telescope" (PDF). Icarus. 137 (2): 260–268. Bibcode:1999Icar..137..260S. doi:10.1006/icar.1999.6047. Retrieved 2005-01-15. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help) [dead link]
  48. ^ "JPL Small-Body Database Browser: 48 Doris". 2008-06-13 last obs. Archived from the original on 2010-01-17. Retrieved 2008-11-10. {{cite web}}: Check date values in: |date= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  49. ^ Millis, R.L (1984). "The diameter of 375 URSULA from its occultation of AG + 39 deg 303". Astronomical Journal. 89: 592–596. Bibcode:1984AJ.....89..592M. doi:10.1086/113553. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  50. ^ Durech., J.; Kaasalainen, M., Marciniak, A.; et al., “Physical models of ten asteroids from an observers' collaboration network”, Astronomy and Astrophysics, Volume 465, Issue 1, April I 2007, pp. 331-337
  51. ^ Stansberry, Grundy, Brown, Spencer, Trilling, Cruikshank, Luc Margot Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope (2007) Preprint arXiv
  52. ^ [Planetary occultations: 2001 results|http://occsec.wellington.net.nz/planet/2001/plnres01.htm#Aurora]
  53. ^ Fernandes, Yanga R. (2003). "The albedo distribution of Jovian Trojan asteroids". The Astronomical Journal. 126 (3): 1563–1574. Bibcode:2003AJ....126.1563F. doi:10.1086/377015. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  54. ^ "JPL Small-Body Database Browser: 7 Iris". 2009-03-17 last obs. Retrieved 2009-03-17. {{cite web}}: Check date values in: |date= (help)
  55. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  56. ^ Davies, J. K.; Tholen, D. J.; Ballantyne, D. R. (1996). "Infrared Observations of Distant Asteroids". Completing the Inventory of the Solar System, Astronomical Society of the Pacific Conference Proceedings. 107: 97–105. Bibcode:1996ciss.conf...97D.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  57. ^ a b c Grundy, W.M. (2007). "The orbit, mass, size, albedo, and density of (65489) Ceto/Phorcys: A tidally-evolved binary Centaur". Icarus. 191 (1): 286. arXiv:0704.1523. Bibcode:2007Icar..191..286G. doi:10.1016/j.icarus.2007.04.004. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help) Cite error: The named reference "Grundy2007" was defined multiple times with different content (see the help page).
  58. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  59. ^ a b (Note, he assumed geometric albedo of 0.04-->) Sheppard, S. S., Jewitt, D. C., Porco, C.; Jupiter's Outer Satellites and Trojans, in Jupiter: The Planet, Satellites and Magnetosphere, edited by Fran Bagenal, Timothy E. Dowling, William B. McKinnon, Cambridge Planetary Science, Vol. 1, Cambridge, UK: Cambridge University Press, ISBN 978-0-521-81808-7, 2004, pp. 263-280 [dead link]
  60. ^ Emelyanov, N.V. (2005). "The mass of Himalia from the perturbations on other satellites". Astronomy and Astrophysics. 438 (3): L33–L36. Bibcode:2005A&A...438L..33E. doi:10.1051/0004-6361:200500143. {{cite journal}}: |access-date= requires |url= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  61. ^ http://www.cfa.harvard.edu/iau/lists/NumberedMPs.txt Template:WebCite
  62. ^ Thomas, P.C. (1998). "The Small Inner Satellites of Jupiter". Icarus. 135 (1): 360–371. Bibcode:1998Icar..135..360T. doi:10.1006/icar.1998.5976. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  63. ^ Anderson, J.D. (2005). "Amalthea's Density Is Less Than That of Water". Science. 308 (5726): 1291–1293. Bibcode:2005Sci...308.1291A. doi:10.1126/science.1110422. PMID 15919987. Archived from the original on 2007-06-28. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  64. ^ a b Descamps, P. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  65. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  66. ^ JPL Small-Body Database Browser on 20461 Dioretsa
  67. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2007-06-23. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  68. ^ "JPL Small-Body Database Browser: 14 Irene". 2008-04-14 last obs. Retrieved 2008-11-27. {{cite web}}: Check date values in: |date= (help)
  69. ^ "Dwarf planet Eris bigger than Pluto - Astronomy Magazine". Astronomy.com. 2007-06-14. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  70. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  71. ^ JPL 508 Template:WebCite
  72. ^ Johnston's Archive about (66652) Borasisi and Pabu
  73. ^ "(212) Médée." Wikipédia, l'encyclopédie libre. 16 jan 2009, 21:16 UTC. 13 mar 2009, 00:01 <http://fr.wikipedia.org/w/index.php?title=(212)_M%C3%A9d%C3%A9e&oldid=37119259>.
  74. ^ "JPL Small-Body Database Browser: 92 Undina". Archived from the original on 2010-01-17. Retrieved 2010-10-09. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  75. ^ Michalak, G. (2001). "Determination of asteroid masses". Astronomy & Astrophysics. 374 (2): 703–711. Bibcode:2001A&A...374..703M. doi:10.1051/0004-6361:20010731. Retrieved 2008-11-10.
  76. ^ Bange, J.F (1997). "DETERMINATION OF THE MASSES OF MINOR PLANETS" (PDF): 169. Retrieved 2008-11-10. {{cite journal}}: Cite journal requires |journal= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  77. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  78. ^ Spitale, J. N.; et al. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal. 132 (2): 692–710. Bibcode:2006AJ....132..692S. doi:10.1086/505206. Archived from the original on 2011-02-12. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  79. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  80. ^ Jonathan Amos - Asteroid Lutetia has thick blanket of debris (4 October 2010) - BBC News Template:WebCite
  81. ^ average of values taken from: H. A. Weaver (2006). "Discovery of two new satellites of Pluto". Nature. 439 (7079): 943–945. arXiv:astro-ph/0601018. Bibcode:2006Natur.439..943W. doi:10.1038/nature04547. PMID 16495991. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |month= ignored (help)
  82. ^ "IRAS Minor Planet Survey". Archived from the original on 2005-12-11.
  83. ^ a b "(90) Antiope and S/2000 (90) 1". Johnstonsarchive.net. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  84. ^ a b c Planetary Satellite Physical Parameters - NASA - 2011
  85. ^ "JPL Small-Body Database Browser: 60558 Echeclus (2000 EC98)". 2008-05-07 last obs. Retrieved 2008-09-09. {{cite web}}: Check date values in: |date= (help)
  86. ^ Tedesco; et al. (2004). "Supplemental IRAS Minor Planet Survey (SIMPS)". IRAS-A-FPA-3-RDR-IMPS-V6.0. Planetary Data System. Archived from the original on 2010-01-17. Retrieved December 31, 2008. {{cite web}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  87. ^ "JPL Small-Body Database Browser: 84 Klio". 2008-03-30 last obs. Retrieved 2008-11-06. {{cite web}}: Check date values in: |date= (help)
  88. ^ Grundy, W. M (2005). "Diverse albedos of small trans-neptunian objects". Icarus. 176 (1): 184–191. arXiv:astro-ph/0502229. Bibcode:2005Icar..176..184G. doi:10.1016/j.icarus.2005.01.007. {{cite journal}}: |access-date= requires |url= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help) (Preprint on arXiv.)
  89. ^ Barucci, M. A., de Bergh, C., Cuby, J.-G., Le Bras, A., Schmitt, B., & Romon, J. (2000). "Infrared spectroscopy of the Centaur 8405 Asbolus: first observations at ESO-VLT". Astronomy and Astrophysics. 357: L53–L56. Bibcode:2000A&A...357L..53B. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)CS1 maint: multiple names: authors list (link)
  90. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  91. ^ Near-infrared spectra of centaurs and Kuiper belt objects
  92. ^ "JPL Small-Body Database Browser: C/1995 O1 (Hale-Bopp)". 2007-10-22 last obs. Retrieved 2008-12-05. {{cite web}}: Check date values in: |date= (help)
  93. ^ Lionel Wilson and Klaus Keil (1991). "Explosive Eruptions on Asteroids: The Missing Basalts on the Aubrite Parent Body". Abstracts of the Lunar and Planetary Science Conference. 22: 1515. Bibcode:1991LPI....22.1515W.
  94. ^ "2008-07-16 Tracking News". Hohmanntransfer.com. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  95. ^ Pierre Vingerhoets and Jan Van Gestel (2004-01-31). "E.A.O.N. : (4348) Poulydamas". European Asteroidal Occultation Network (E.A.O.N.). Archived from the original on 2011-02-12. Retrieved 2010-05-31. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  96. ^ Thomas, P.C. (1998). "The Small Inner Satellites of Jupiter". ICARUS. 135 (1): 360–371. Bibcode:1998Icar..135..360T. doi:10.1006/icar.1998.5976. Archived from the original on 2011-02-12. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  97. ^ Britt et al. 2002, p. 486
  98. ^ Attention: This template ({{cite doi}}) is deprecated. To cite the publication identified by doi:10.1006/icar.2001.6597, please use {{cite journal}} (if it was published in a bona fide academic journal, otherwise {{cite report}} with |doi=10.1006/icar.2001.6597 instead.
  99. ^ a b c Porco, C. C.; et al. (2007). "Saturn's Small Inner Satellites: Clues to Their Origins". Science. 318 (5856): 1602–1607. Bibcode:2007Sci...318.1602P. doi:10.1126/science.1143977. PMID 18063794. Archived from the original on 2011-02-12. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  100. ^ F. Marchis; et al. (2003). "A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope". Icarus. 165 (1): 112. Bibcode:2003Icar..165..112M. doi:10.1016/S0019-1035(03)00195-7. Archived from the original on 2011-02-12. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  101. ^ Porco, C.C.; et al. (2006). "Physical Characteristics and Possible Accretionary Origins for Saturn's Small Satellites". Bulletin of the American Astronomical Society. 37: 768. Archived from the original (PDF) on 2007-07-27. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  102. ^ IOTA/IOTA-ES occultation update for (2000) Herschel
  103. ^ JPL Small-Body Database Browser: 2000 Herschel
  104. ^ "JPL Small-Body Database Browser: 65407 (2002 RP120)". Archived from the original on 2011-02-12. Retrieved 2008-02-06. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  105. ^ "The Shape of Gaspra : Galileo's observations of 951 Gaspra". Cat.inist.fr. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  106. ^ a b F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813. Archived from the original on 2011-02-12. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  107. ^ 11 km average diameter 2004 study 1P at the JPL Small-Body Database Edit this at Wikidata
  108. ^ Using the volume of an ellipsoid of 15x8x8km * an assumed rubble pile density of 0.6 g/cm3 yields a mass (m=d*v) of ~3.02E+14 kg
  109. ^ Scott S. Sheppard. "Uranus' Known Satellites". Carnegie Institution (Department of Terrestrial Magnetism). Retrieved 2011-01-22.
  110. ^ Porco, C. C.; et al. (2007). "Saturn's Small Inner Satellites: Clues to Their Origins". Science. 318 (5856): 1602–1607. Bibcode:2007Sci...318.1602P. doi:10.1126/science.1143977. PMID 18063794. Archived from the original on 2011-02-12. {{cite journal}}: Explicit use of et al. in: |author= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  111. ^ "Comet 9P/Tempel 1". The Planetary Society. Archived from the original on 2011-02-12. Retrieved 2008-12-16. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  112. ^ "JPL Small-Body Database Browser: 9P/Tempel 1". 2008-10-25 last obs. Archived from the original on 2011-02-12. Retrieved 2008-12-16. {{cite web}}: Check date values in: |date= (help); Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  113. ^ Cassini Equinox Mission: Thrym (accessed October 2010) Template:WebCite
  114. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  115. ^ "Jupiter, in Astronomy"; The Columbia Encyclopedia, Sixth Edition, 2004. 52323 pgs.
  116. ^ H. U. Keller, et all - E-Type Asteroid (2867) Steins as Imaged by OSIRIS on Board Rosetta - Science 8 January 2010: Vol. 327. no. 5962, pp. 190 - 193 DOI: 10.1126/science.1179559 [dead link]
  117. ^ 4.8 km diameter 19P/Borrelly at the JPL Small-Body Database Edit this at Wikidata
  118. ^ 2P/Encke at the JPL Small-Body Database Edit this at Wikidata
  119. ^ C/1996 B2 at the JPL Small-Body Database Edit this at Wikidata
  120. ^ "Comet Hyakutake Home Page (JPL)". .jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  121. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  122. ^ Source: Porco et al. 2005 Template:WebCite
  123. ^ "Cloudbait Observatory Gallery - Comet Holmes". Cloudbait.com. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  124. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  125. ^ 6178 (1986 DA) at the JPL Small-Body Database Edit this at Wikidata
  126. ^ a b Roman Numerals
  127. ^ Tedesco, Edward (April 4, 2002). "New study reveals twice as many asteroids as previously believed" (Press release). European Space Agency. Retrieved 2009-10-20. {{cite press release}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  128. ^ Minor Planet No. 100,000 Named for Space Age 50th Anniversary (2007) - Space Ref, Quote: "..about a mile in size"
  129. ^ [JPL Small-Body Database Browser: 100000 Astronautica]
  130. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  131. ^ "(4769) Castalia." Wikipédia, l'encyclopédie libre. 20 jan 2010, 16:37 UTC. 11 oct 2010, 16:48 <http://fr.wikipedia.org/w/index.php?title=(4769)_Castalia&oldid=49048108>
  132. ^ 3000 x 10^9 kg
  133. ^ a b Lisse, C. M. (2009). "Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2". Publications of the Astronomical Society of the Pacific. 121: 968–975. Bibcode:2009PASP..121..968L. doi:10.1086/605546. {{cite journal}}: Cite has empty unknown parameter: |1= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  134. ^ "JPL Small-Body Database Browser: 14827 Hypnos (1986 JK)". Archived from the original on 2011-02-12. Retrieved 2008-02-08. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  135. ^ Whitman, Kathryn (2006). "The Size-Frequency Distribution of Dormant Jupiter Family Comets". arXiv:astro-ph/0603106. Bibcode:2006Icar..183..101W. doi:10.1016/j.icarus.2006.02.016. {{cite journal}}: Cite journal requires |journal= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  136. ^ 2062 Aten (this version) [dead link]
  137. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  138. ^ a b c Based on an assumed density of 2.6 g/cm3 as given at the NASA NEO impact risk page http://neo.jpl.nasa.gov/risk/index.html Template:WebCite
  139. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  140. ^ BBC - Giant asteroid passes near Earth - 9 November 2011
  141. ^ The Herschel Space Observatory catches a glimpse of the minor planet during its rendezvous with Earth (November 17, 2011)
  142. ^ JPL Small-Body Database Browser (2005 YU55)
  143. ^ "NASA Scientists Get First Images of Earth Flyby Asteroid". NASA/JPL. 2008-01-25. Archived from the original on 2011-02-12. Retrieved 2008-01-26. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  144. ^ [http://neo.jpl.nasa.gov/risk/1994wr12.html NASA - 1994 WR12 Earth Impact Risk Summary - 2011]
  145. ^ a b c BBC News - Record spin for newfound asteroid (2008) Template:WebCite
  146. ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)

Further reading

External links

Template:Link FL