866 Fatme: Difference between revisions

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{{Use dmy dates|date=March 2020}}
{{Infobox planet
{{Infobox planet
| minorplanet= yes
| minorplanet = yes
| name = 866 Fatme
| background= #D6D6D6
| background = #D6D6D6
| name= 866 Fatme
| image =
| mpc_name= (866) Fatme
| image_size =
| alt_names= 1917 BQ
| caption =
| discoverer= [[Max Wolf]]
| discovery_ref = &thinsp;<ref name="MPC-object" />
| discovered= 25 February 1917
| discovery_site= [[Heidelberg]]
| discoverer = [[Max Wolf|M. F. Wolf]]
| discovery_site = [[Heidelberg-Königstuhl State Observatory|Heidelberg Obs.]]
| epoch= 31 July 2016 ([[Julian day|JD]] 2457600.5)
| discovered = 25 February 1917
| eccentricity= 0.054693
| mpc_name = (866) Fatme
| semimajor= {{Convert|3.1247|AU|Gm|abbr=on}}
| alt_names = A917 DG{{·}}{{mp|1950 DF|1}}<br />1917 BQ
| perihelion= {{Convert|2.9538|AU|Gm|abbr=on}}
| pronounced =
| aphelion= {{Convert|3.2956|AU|Gm|abbr=on|lk=on}}
| named_after = Fatme, a character in the opera ''[[Abu Hassan]]''<br />{{small|([[Carl Maria von Weber]])}}<ref name="springer" />
| period= 5.52 [[Julian year (astronomy)|yr]] (2017.4 [[Julian year (astronomy)|d]])
| mp_category = [[main-belt]]&thinsp;<ref name="MPC-object" /><ref name="jpldata" />{{·}}{{small|([[Kirkwood gap|outer]])}}<br />[[Background asteroid|background]]&thinsp;<ref name="AstDys-object" /><ref name="Ferret" />
| inclination= 8.6468°
| orbit_ref = &thinsp;<ref name="jpldata" />
| asc_node= 91.282°
| epoch = 31 May 2020 ([[Julian day|JD]] 2459000.5)
| arg_peri= 259.517°
| uncertainty = 0
| mean_anomaly= 148.521[[Degree (angle)|°]]
| observation_arc = 102.93 [[Julian year (astronomy)|yr]] (37,596 d)
| mean_motion= {{Deg2DMS|0.17844|sup=ms}} / day
| aphelion = 3.2871 [[Astronomical unit|AU]]
| orbit_ref= <ref name="jpldata">{{Cite web |url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=866;cad=1 |title=866 Fatme (1917 BQ) |work=[[JPL Small-Body Database]] |publisher=[[NASA]]/[[Jet Propulsion Laboratory]] |access-date=4 May 2016}}</ref>
| perihelion = 2.9606 AU
| observation_arc= 99.09 yr (36192 days)
| semimajor = 3.1238 AU
| uncertainty= 0
| abs_magnitude= 9.6
| eccentricity = 0.0523
| period = 5.52 yr (2,017 d)
| rotation= {{Convert|20.03|h|d|abbr=on|lk=on}}
| mean_anomaly = 34.544[[Degree (angle)|°]]
| albedo= {{val|0.0473|0.002}}
| mean_radius= {{val|44.155|1}} [[Kilometre|km]]
| mean_motion = {{Deg2DMS|0.1785|sup=ms}} / day
| inclination = 8.6616°
| moid= {{Convert|1.96223|AU|Gm|abbr=on}}
| asc_node = 91.060°
| jupiter_moid= {{Convert|1.97815|AU|Gm|abbr=on}}
| tisserand= 3.195
| arg_peri = 263.20°
| mean_diameter = {{plainlist|
* {{val|78.061|0.360|ul=km}}<ref name="Mainzer-2016" /><ref name="Masiero-2014" />
* {{val|86.49|1.16|u=km}}<ref name="AKARI" />
* {{val|88.31|2.0|u=km}}<ref name="SIMPS" />}}
| rotation = {{val|5.800|0.002|ul=h}}<ref name="Polakis-2018e" />
| albedo = {{plainlist|
* {{val|0.038|0.001}}<ref name="AKARI" />
* {{val|0.046|0.007}}<ref name="Mainzer-2016" /><ref name="Masiero-2014" />
* {{val|0.0473|0.002}}<ref name="SIMPS" />}}
| spectral_type = [[SMASS classification|SMASS]] {{=}} [[X-type asteroid|X]]&thinsp;<ref name="jpldata" />
| abs_magnitude = 9.50<ref name="MPC-object" /><ref name="jpldata" />
}}
}}


'''866 Fatme''' (''[[Minor planet provisional designation|prov. designation]]:'' {{mp|A917 DG}} ''or'' {{mp|1917 BQ}}) is a large [[background asteroid]], approximately {{convert|86|km|mi|abbr=off|sigfig=2|sp=us}} in diameter, located in the outer region of the [[asteroid belt]]. It was discovered by German astronomer [[Max Wolf]] at the [[Heidelberg-Königstuhl State Observatory]] on 25 February 1917.<ref name="MPC-object" /> The [[X-type asteroid]] has a short [[rotation period]] of 5.8 hours. It was named after "Fatme", a character in the opera ''[[Abu Hassan]]'' by [[Carl Maria von Weber]] (1786–1826).<ref name="springer" />
'''866 Fatme''' is a [[minor planet]] orbiting the [[Sun]]. It was named after Fatme, a character in [[Carl Maria von Weber]]'s opera ''[[Abu Hassan]]''.

== Orbit and classification ==

''Fatme'' is a non-[[Asteroid family|family]] asteroid of the main belt's [[Background asteroid|background population]] when applying the [[hierarchical clustering method]] to its [[proper orbital elements]].<ref name="AstDys-object" /><ref name="Ferret" /> It orbits the Sun in the [[Kirkwood gap|outer]] asteroid belt at a distance of 3.0–3.3&nbsp;[[Astronomical unit|AU]] once every 5 years and 6 months (2,017 days; [[semi-major axis]] of 3.12&nbsp;AU). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.05 and an [[orbital inclination|inclination]] of 9[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" /> The body's [[observation arc]] begins at [[Heidelberg Observatory]] on 16 March 1917, or three weeks after its official discovery observation.<ref name="MPC-object" />

== Naming ==

This [[minor planet]] was named after Fatme, a character in the opera ''[[Abu Hassan]]'' by German composer [[Carl Maria von Weber]] (1786–1826). The official {{MoMP|866|naming}} was also mentioned in ''[[The Names of the Minor Planets]]'' by [[Paul Herget]] in 1955 ({{small|[[Herget's discovery circumstances|H 85]]}}).<ref name="springer" /> Another asteroid [[865&nbsp;Zubaida]], was also named after a character of this opera. The composer himself was honored with the naming of [[4152&nbsp;Weber]].

== Physical characteristics ==

In the Bus–Binzel [[SMASS classification]], ''Fatme'' is an [[X-type asteroid]].<ref name="jpldata" />

=== Rotation period ===

In June 2018, a rotational [[lightcurve]] of ''Fatme'' was obtained from 5 nights of [[Photometry (astronomy)|photometric]] observations by [[Thomas A. Polakis|Tom Polakis]] at the Command Module Observatory {{Obscode|V02}} in Arizona. Lightcurve analysis gave a [[rotation period]] of {{val|5.800|0.002}} hours with a brightness variation of {{val|0.21|0.02}} [[Magnitude (astronomy)|magnitude]] ({{small|[[LCDB quality code|U=2]]}}).<ref name="Polakis-2018e" /> The result supersedes previously reported period determinations of {{val|20.03|0.01}} hours with an amplitude of {{val|0.21|0.05}} magnitude by [[Robert D. Stephens|Robert Stephens]] at the Santana Observatory {{Obscode|646}}, California, in May 2001 ({{small|[[LCDB quality code|U=2]]}}),<ref name="Stephens-2002a" /> {{val|9.4|0.2}} hours with an amplitude of {{val|0.06|0.01}} magnitude (tentative) by French amateur astronomer [[Laurent Bernasconi]] in December 2004 ({{small|[[LCDB quality code|U=1]]}}),<ref name="geneva-obs" /> {{val|9.36|0.05}} hours with an amplitude of {{val|0.06|0.01}} magnitude (tentative) by French amateur astronomer [[René Roy (astronomer)|René Roy]] in May 2012 ({{small|[[LCDB quality code|U=2−]]}}),<ref name="geneva-obs" /> and {{val|20.7|0.1}} hours with an amplitude of {{val|0.12|0.02}} magnitude by the Spanish group of asteroid observers, OBAS, in January 2016 ({{small|[[LCDB quality code|U=2−]]}}).<ref name="Aznar-2016c" />

=== Diameter and albedo ===

According to the surveys carried out by the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]] (WISE), the Japanese [[Akari (satellite)|Akari satellite]], and the Infrared Astronomical Satellite [[IRAS]], ''Fatme'' measures ({{val|78.061|0.360}}), ({{val|86.49|1.16}}) and ({{val|88.31|2.0}}) kilometers in diameter and its surface has an [[astronomical albedo|albedo]] of ({{val|0.046|0.007}}), ({{val|0.038|0.001}}) and ({{val|0.0473|0.002}}), respectively.<ref name="Mainzer-2016" /><ref name="Masiero-2014" /><ref name="SIMPS" /><ref name="AKARI" /> The ''Collaborative Asteroid Lightcurve Link'' derives an albedo of 0.0361 and a diameter of 88.11 kilometers based on an [[absolute magnitude]] of 9.5.<ref name="lcdb" /> Alternative mean-diameter measurements published by the WISE team include ({{val|82.388|1.055|u=km}}), ({{val|88.25|26.33|u=km}}) and ({{val|95.83|37.32|u=km}}) with corresponding albedos of ({{val|0.0412|0.0096}}), ({{val|0.04|0.03}}) and ({{val|0.03|0.02}}).<ref name="Ferret" /><ref name="lcdb" />


== References ==
== References ==
{{reflist|30em|refs=
{{Reflist}}

<ref name="jpldata">{{cite web
|type = 2020-02-01 last obs.
|title = JPL Small-Body Database Browser: 866 Fatme (A917 DG)
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000866
|publisher = [[Jet Propulsion Laboratory]]
|accessdate = 5 March 2020}}</ref>

<ref name="springer">{{cite book
|title = Dictionary of Minor Planet Names
|last = Schmadel | first = Lutz D.
|publisher = Springer Berlin Heidelberg
|chapter = (866) Fatme
|page = 79
|date = 2007
|doi = 10.1007/978-3-540-29925-7_867
|isbn = 978-3-540-00238-3}}</ref>

<ref name="MPC-object">{{cite web
|title = 866 Fatme (A917 DG)
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=866
|accessdate = 5 March 2020}}</ref>

<ref name="geneva-obs">{{cite web
|title = Asteroids and comets rotation curves – (866) Fatme
|last = Behrend |first = Raoul
|publisher = Geneva Observatory
|url = http://obswww.unige.ch/~behrend/page3cou.html#000866
|accessdate = 5 March 2020}}</ref>

<ref name="Masiero-2014">{{cite journal
|display-authors = 6
|first1 = Joseph R. |last1 = Masiero
|first2 = T. |last2 = Grav
|first3 = A. K. |last3 = Mainzer
|first4 = C. R. |last4 = Nugent
|first5 = J. M. |last5 = Bauer
|first6 = R. |last6 = Stevenson
|first7 = S. |last7 = Sonnett
|date = August 2014
|title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
|journal = The Astrophysical Journal
|volume = 791
|issue = 2
|page = 11
|bibcode = 2014ApJ...791..121M
|doi = 10.1088/0004-637X/791/2/121
|arxiv = 1406.6645}}</ref>

<ref name="Mainzer-2016">{{cite journal
|display-authors = 6
|first1 = A. K. |last1 = Mainzer
|first2 = J. M. |last2 = Bauer
|first3 = R. M. |last3 = Cutri
|first4 = T. |last4 = Grav
|first5 = E. A. |last5 = Kramer
|first6 = J. R. |last6 = Masiero
|first7 = C. R. |last7 = Nugent
|first8 = S. M. |last8 = Sonnett
|first9 = R. A. |last9 = Stevenson
|first10 = E. L. |last10 = Wright
|date = June 2016
|title = NEOWISE Diameters and Albedos V1.0
|url = https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab
|journal = NASA Planetary Data System
|bibcode = 2016PDSS..247.....M
|access-date= 5 March 2020}}</ref>

<ref name="SIMPS">{{cite journal
|first1 = E. F. |last1 = Tedesco
|first2 = P. V. |last2 = Noah
|first3 = M. |last3 = Noah
|first4 = S. D. |last4 = Price
|date = October 2004
|title = IRAS Minor Planet Survey V6.0
|url = https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
|journal = NASA Planetary Data System
|volume = 12
|pages = IRAS-A-FPA-3-RDR-IMPS-V6.0
|bibcode = 2004PDSS...12.....T
|accessdate = 5 March 2020}}</ref>

<ref name="AKARI">{{cite journal
|display-authors = 6
|first1 = Fumihiko |last1 = Usui
|first2 = Daisuke |last2 = Kuroda
|first3 = Thomas G. |last3 = Müller
|first4 = Sunao |last4 = Hasegawa
|first5 = Masateru |last5 = Ishiguro
|first6 = Takafumi |last6 = Ootsubo
|first7 = Daisuke |last7 = Ishihara
|first8 = Hirokazu |last8 = Kataza
|first9 = Satoshi |last9 = Takita
|first10 = Shinki |last10 = Oyabu
|first11 = Munetaka |last11 = Ueno
|first12 = Hideo |last12 = Matsuhara
|first13 = Takashi |last13 = Onaka
|date = October 2011
|title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
|url = http://pasj.oxfordjournals.org/content/63/5/1117.full.pdf+html
|journal = Publications of the Astronomical Society of Japan
|volume = 63
|issue = 5
|pages = 1117–1138
|bibcode = 2011PASJ...63.1117U
|doi = 10.1093/pasj/63.5.1117
|access-date= 5 March 2020}} ([http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-source=J/PASJ/63/1117/acua_v1&Num=866 online], [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153])</ref>

<ref name="lcdb">{{cite web
|title = LCDB Data for (866) Fatme
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=866
|accessdate = 5 March 2020}}</ref>

<ref name="Stephens-2002a">{{cite journal
|last1 = Stephens |first1 = R. D.
|date = March 2002
|title = Photometry of 866 Fatme, 894 Erda, 1108 Demeter, and 3443 Letsungdao
|journal = Minor Planet Bulletin
|url = http://www.minorplanet.info/MPB/issues/MPB_29-1.pdf
|volume = 29
|issue = 1
|pages = 2–3
|bibcode = 2002MPBu...29....2S}}</ref>

<ref name="Aznar-2016c">{{cite journal
|display-authors = 6
|last1 = Aznar Macias |first1 = Amadeo
|last2 = Carreno Garcerain |first2 = Alfonso
|last3 = Arce Masego |first3 = Enrique
|last4 = Brines Rodriguez |first4 = Pedro
|last5 = Lozano de Haro |first5 = Juan
|last6 = Fornas Silva |first6 = Alvaro
|last7 = Fornas Silva |first7 = Gonzalo
|last8 = Mas Martinez |first8 = Vicente
|last9 = Rodrigo Chiner |first9 = Onofre
|last10 = Herrero Porta |first10 = David
|date = July 2016
|title = Twenty-one Asteroid Lightcurves at Group Observadores de Asteroides (OBAS): Late 2015 to Early 2016
|journal = Minor Planet Bulletin
|url = http://www.minorplanet.info/MPB/issues/MPB_43-3.pdf
|volume = 43
|issue = 3
|pages = 257–263
|bibcode = 2016MPBu...43..257A
|issn = 1052-8091}}</ref>

<ref name="Polakis-2018e">{{cite journal
|last1 = Polakis |first1 = Tom
|date = October 2018
|title = Lightcurve Analysis for Fourteen Main-belt Minor Planets
|journal = Minor Planet Bulletin
|url = http://www.minorplanet.info/MPB/issues/MPB_45-4.pdf
|volume = 45
|issue = 4
|pages = 347–352
|bibcode = 2018MPBu...45..347P
|issn = 1052-8091}}</ref>

<ref name="Ferret">{{cite web
|title = Asteroid 866 Fatme
|work = Small Bodies Data Ferret
|url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=866+Fatme
|accessdate = 5 March 2020}}</ref>

<ref name="AstDys-object">{{cite web
|title = Asteroid 866 Fatme – Proper Elements
|publisher = AstDyS-2, Asteroids – Dynamic Site
|url = https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=866
|access-date= 5 March 2020}}</ref>

}} <!-- end of reflist -->


== External links ==
== External links ==
* [http://www.minorplanet.info/PHP/OneAsteroidInfo.php Lightcurve Database Query] (LCDB), at ''www.minorplanet.info''
* [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
* [http://obswww.unige.ch/~behrend/page_cou.html Asteroids and comets rotation curves, CdR] – ''[[Geneva Observatory]]'', [[Raoul Behrend]]
* [http://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
* {{AstDys|866}}
* {{AstDys|866}}
* {{JPL small body}}
* {{JPL small body}}


{{Use dmy dates|date=October 2019}}
{{Minor planets navigator |865 Zubaida |number=866 |867 Kovacia}}
{{Minor planets navigator |865 Zubaida |number=866 |867 Kovacia}}
{{Small Solar System bodies}}
{{Small Solar System bodies}}
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[[Category:X-type asteroids (SMASS)|000866]]
[[Category:X-type asteroids (SMASS)|000866]]
[[Category:Astronomical objects discovered in 1917|19170225]]
[[Category:Astronomical objects discovered in 1917|19170225]]


{{beltasteroid-stub}}

Revision as of 03:36, 5 March 2020

866 Fatme
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date25 February 1917
Designations
(866) Fatme
Named after
Fatme, a character in the opera Abu Hassan
(Carl Maria von Weber)[2]
A917 DG · 1950 DF1
1917 BQ
main-belt[1][3] · (outer)
background[4][5]
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc102.93 yr (37,596 d)
Aphelion3.2871 AU
Perihelion2.9606 AU
3.1238 AU
Eccentricity0.0523
5.52 yr (2,017 d)
34.544°
0° 10m 42.6s / day
Inclination8.6616°
91.060°
263.20°
Physical characteristics
Mean diameter
5.800±0.002 h[10]
SMASS = X[3]
9.50[1][3]

866 Fatme (prov. designation: A917 DG or 1917 BQ) is a large background asteroid, approximately 86 kilometers (53 miles) in diameter, located in the outer region of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 25 February 1917.[1] The X-type asteroid has a short rotation period of 5.8 hours. It was named after "Fatme", a character in the opera Abu Hassan by Carl Maria von Weber (1786–1826).[2]

Orbit and classification

Fatme is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the outer asteroid belt at a distance of 3.0–3.3 AU once every 5 years and 6 months (2,017 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.05 and an inclination of 9° with respect to the ecliptic.[3] The body's observation arc begins at Heidelberg Observatory on 16 March 1917, or three weeks after its official discovery observation.[1]

Naming

This minor planet was named after Fatme, a character in the opera Abu Hassan by German composer Carl Maria von Weber (1786–1826). The official naming was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 85).[2] Another asteroid 865 Zubaida, was also named after a character of this opera. The composer himself was honored with the naming of 4152 Weber.

Physical characteristics

In the Bus–Binzel SMASS classification, Fatme is an X-type asteroid.[3]

Rotation period

In June 2018, a rotational lightcurve of Fatme was obtained from 5 nights of photometric observations by Tom Polakis at the Command Module Observatory (V02) in Arizona. Lightcurve analysis gave a rotation period of 5.800±0.002 hours with a brightness variation of 0.21±0.02 magnitude (U=2).[10] The result supersedes previously reported period determinations of 20.03±0.01 hours with an amplitude of 0.21±0.05 magnitude by Robert Stephens at the Santana Observatory (646), California, in May 2001 (U=2),[11] 9.4±0.2 hours with an amplitude of 0.06±0.01 magnitude (tentative) by French amateur astronomer Laurent Bernasconi in December 2004 (U=1),[12] 9.36±0.05 hours with an amplitude of 0.06±0.01 magnitude (tentative) by French amateur astronomer René Roy in May 2012 (U=2−),[12] and 20.7±0.1 hours with an amplitude of 0.12±0.02 magnitude by the Spanish group of asteroid observers, OBAS, in January 2016 (U=2−).[13]

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Japanese Akari satellite, and the Infrared Astronomical Satellite IRAS, Fatme measures (78.061±0.360), (86.49±1.16) and (88.31±2.0) kilometers in diameter and its surface has an albedo of (0.046±0.007), (0.038±0.001) and (0.0473±0.002), respectively.[6][7][9][8] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0361 and a diameter of 88.11 kilometers based on an absolute magnitude of 9.5.[14] Alternative mean-diameter measurements published by the WISE team include (82.388±1.055 km), (88.25±26.33 km) and (95.83±37.32 km) with corresponding albedos of (0.0412±0.0096), (0.04±0.03) and (0.03±0.02).[5][14]

References

  1. ^ a b c d e "866 Fatme (A917 DG)". Minor Planet Center. Retrieved 5 March 2020.
  2. ^ a b c Schmadel, Lutz D. (2007). "(866) Fatme". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 79. doi:10.1007/978-3-540-29925-7_867. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f "JPL Small-Body Database Browser: 866 Fatme (A917 DG)" (2020-02-01 last obs.). Jet Propulsion Laboratory. Retrieved 5 March 2020.
  4. ^ a b "Asteroid 866 Fatme – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 5 March 2020.
  5. ^ a b c "Asteroid 866 Fatme". Small Bodies Data Ferret. Retrieved 5 March 2020.
  6. ^ a b c Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. Bibcode:2016PDSS..247.....M. Retrieved 5 March 2020.
  7. ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
  8. ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 5 March 2020. (online, AcuA catalog p. 153)
  9. ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 5 March 2020.
  10. ^ a b Polakis, Tom (October 2018). "Lightcurve Analysis for Fourteen Main-belt Minor Planets" (PDF). Minor Planet Bulletin. 45 (4): 347–352. Bibcode:2018MPBu...45..347P. ISSN 1052-8091.
  11. ^ Stephens, R. D. (March 2002). "Photometry of 866 Fatme, 894 Erda, 1108 Demeter, and 3443 Letsungdao" (PDF). Minor Planet Bulletin. 29 (1): 2–3. Bibcode:2002MPBu...29....2S.
  12. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (866) Fatme". Geneva Observatory. Retrieved 5 March 2020.
  13. ^ Aznar Macias, Amadeo; Carreno Garcerain, Alfonso; Arce Masego, Enrique; Brines Rodriguez, Pedro; Lozano de Haro, Juan; Fornas Silva, Alvaro; et al. (July 2016). "Twenty-one Asteroid Lightcurves at Group Observadores de Asteroides (OBAS): Late 2015 to Early 2016" (PDF). Minor Planet Bulletin. 43 (3): 257–263. Bibcode:2016MPBu...43..257A. ISSN 1052-8091.
  14. ^ a b "LCDB Data for (866) Fatme". Asteroid Lightcurve Database (LCDB). Retrieved 5 March 2020.

External links