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{{Infobox planet
{{Infobox planet
| minorplanet = yes
| minorplanet = yes
| mpc_name = (1153) Wallenbergia
| name = 1153 Wallenbergia
| background = #FFFFC0
| background = #D6D6D6
| image =
| name = 1153 Wallenbergia&thinsp;<ref name="a">{{cite web | title=JPL Small-Body Database Browser | url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1153 | accessdate= 1 May 2016 }}</ref>
| image_size =
| discoverer = Belyavskij, S.
| caption =
| discovered = 5 September 1924
| discovery_ref = &thinsp;<ref name="jpldata" />
| epoch = 31 July 2016 ([[Julian day|JD]] 2457600.5)
| discoverer = [[Sergey Belyavsky|S. Belyavskyj]]
| aphelion = {{Convert|2.5488687|AU|Gm|abbr=on|lk=on}}
| discovery_site = [[Simeiz Observatory|Simeiz Obs.]]
| perihelion = {{Convert|1.8421363|AU|Gm|abbr=on}}
| discovered = 5 September 1924
| semimajor = {{Convert|2.1955025|AU|Gm|abbr=on}}
| mpc_name = (1153) Wallenbergia
| eccentricity = 0.1609500
| alt_names = 1924 SL{{·}}1930 HH
| period = 3.25 [[Julian year (astronomy)|yr]] (1188.2 [[Julian year (astronomy)|d]])
| pronounced =
| inclination = 3.334877°
| named_after = Georg Wallenberg&thinsp;<ref name="springer" />{{efn|name=DoMPN-middle-name}}<br />{{small|(German mathematician)}}
| asc_node = 280.55527°
| mp_category = [[main-belt]]{{·}}{{small|([[Kirkwood gap|inner]])}}{{·}}[[Flora family|Flora]]&thinsp;<ref name="lcdb" />
| mean_anomaly = 116.24515[[Degree (angle)|°]]
| orbit_ref = &thinsp;<ref name="jpldata" />
| arg_peri = 28.831152°
| epoch = 4 September 2017 ([[Julian day|JD]] 2458000.5)
| abs_magnitude = 12.1
| uncertainty = 0
| rotation = {{Convert|4.096|h|d|abbr=on|lk=on}}
| observation_arc = 87.02 yr (31,784 days)
| mean_motion = {{Deg2DMS|0.3029725|sup=ms}} / day
| aphelion = 2.5489 [[Astronomical unit|AU]]
| orbit_ref = &thinsp;<ref name="a" />
| perihelion = 1.8428 AU
| observation_arc = 85.79 yr (31333 days)
| semimajor = 2.1958 AU
| uncertainty = 0
| eccentricity = 0.1608
| moid = {{Convert|0.827866|AU|Gm|abbr=on}}
| period = 3.25 [[Julian year (astronomy)|yr]] (1,189 days)
| jupiter_moid = {{Convert|2.68081|AU|Gm|abbr=on}}
| mean_anomaly = 237.52[[Degree (angle)|°]]
| tisserand = 3.650
| mean_motion = {{Deg2DMS|0.3029|sup=ms}} / day
| inclination = 3.3345°
| asc_node = 280.54°
| arg_peri = 28.766°
| dimensions = {{val|8.02|1.81}} km<ref name="Nugent-2016" /><br />{{val|8.037|0.357}} km<ref name="Masiero-2012" /><br />9.36 km {{small|(derived)}}<ref name="lcdb" />
| rotation = {{val|4.096|0.002}} [[Hour|h]]<ref name="Wisniewski-1997" /><br />{{val|4.116|0.0055}} h<ref name="Waszczak-2015" /><br />{{val|4.12|0.070}} h<ref name="Chang-2015" />
| albedo = 0.24 {{small|(assumed)}}<ref name="lcdb" /><br />{{val|0.37|0.14}}<ref name="Nugent-2016" /><br />{{val|0.433|0.091}}<ref name="Masiero-2012" />
| spectral_type = [[S-type asteroid|S]]&thinsp;<ref name="lcdb" /><ref name="Veres-2015" />
| abs_magnitude = {{val|11.985|0.002}} {{small|(R)}}<ref name="Waszczak-2015" />{{·}}12.00<ref name="Masiero-2012" />{{·}}{{val|12.040|0.100}} {{small|(R)}}<ref name="Chang-2015" />{{·}}12.1<ref name="jpldata" />{{·}}12.28<ref name="Nugent-2016" />{{·}}{{val|12.31|0.08}}<ref name="lcdb" /><ref name="Wisniewski-1997" /><ref name="Pravec-2012b" />{{·}}{{val|12.49|0.22}}<ref name="Veres-2015" />
}}
}}


'''1153 Wallenbergia''' is a [[main belt asteroid]] orbiting the [[Sun]]. It makes a revolution around the Sun once every 3 years. It completes one rotation once every 4 hours. It was discovered by [[Sergei Ivanovich Belyavsky]] at [[Simeis]] on September 5, 1924.<ref name="a"/> It was named for the German mathematician [[Georg James Wallenberg]]. Its provisional designation was 1924 SL.<ref>{{cite book |last= Schmadel |first= Lutz D. |title= Dictionary of Minor Planet Names |publisher= Springer |date= 2003 |isbn= 3-540-00238-3 }}</ref>
'''1153 Wallenbergia''', provisional designation {{mpf|1924 SL}}, is a stony Florian [[asteroid]] from the inner regions of the [[asteroid belt]], approximately 8 kilometers in diameter. It was discovered on 5 September 1924, by Soviet astronomer [[Sergey Belyavsky]] at the [[Simeiz Observatory]] on the Crimean peninsula.<ref name="MPC-object" /> The asteroid was named after German mathematician [[Georg Wallenberg]].<ref name="springer" />


== Orbit and classification ==
==References==
{{Reflist}}


''Wallenbergia'' is a member of the [[Flora family]] ({{small|[[FIN tbl#402|402]]}}), a giant [[asteroid family]] and the largest family of stony asteroids in the main-belt.<ref name="lcdb" /> It orbits the Sun in the [[Kirkwood gap|inner]] main-belt at a distance of 1.8–2.5&nbsp;[[Astronomical unit|AU]] once every 3 years and 3 months (1,189 days). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.16 and an [[orbital inclination|inclination]] of 3[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" />
==External links==

The body's [[observation arc]] begins with its identification as {{mpf|1930 HH}} at [[Johannesburg Observatory]] in April 1930, almost six years after its official discovery observation at Simeiz.<ref name="MPC-object" />

== Physical characteristics ==

''Wallenbergia'' has been characterized as a stony [[S-type asteroid]] by [[PanSTARRS]] photometric survey.<ref name="Veres-2015" />

=== Rotation period ===

In September 1989, the first rotational [[lightcurve]] of ''Wallenbergia'' was obtained from photometric observations by Polish astronomer [[Wiesław Z. Wiśniewski]] at [[University of Arizona]]. Lightcurve analysis gave a well-defined [[rotation period]] of 4.096 hours with a brightness amplitude of 0.33 [[Magnitude (astronomy)|magnitude]] ({{small|[[LCDB quality code|U=3]]}}).<ref name="Wisniewski-1997" /> Observations in the R-band at the [[Palomar Transient Factory]] in 2012, gave a period of 4.116 and 4.12 hours with an amplitude of 0.25 and 0.23 magnitude, respectively ({{small|[[LCDB quality code|U=2/2]]}}).<ref name="Waszczak-2015" /><ref name="Chang-2015" />

=== Diameter and albedo ===

According to the survey carried out by the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]], ''Wallenbergia'' measures 8.02 and 8.037 kilometers in diameter and its surface has an [[astronomical albedo|albedo]] of 0.37 and 0.433, respectively.<ref name="Nugent-2016" /><ref name="Masiero-2012" />

The ''Collaborative Asteroid Lightcurve Link'' assumes an albedo of 0.24 – taken from [[8&nbsp;Flora]], the parent body of the Flora family – and derives a diameter of 9.36 kilometers based on an [[absolute magnitude]] of 12.31.<ref name="lcdb" />

== Naming ==

This [[minor planet]] was named after German mathematician Georg Wallenberg (1864–1924). The official naming citation was mentioned in ''[[The Names of the Minor Planets]]'' by [[Paul Herget]] in 1955 ({{small|[[Herget's discovery circumstances|H 107]]}}).<ref name="springer" />{{efn|name=DoMPN-middle-name}}

== Notes ==
{{notelist|refs=

{{efn|name=DoMPN-middle-name|1=Wallenberg's middle name is likely "Jakob", not "James" as given in the ''Dictionary of Minor Planet Names''}}

}} <!-- end of notelist -->

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

<ref name="jpldata">{{cite web
|type = 2017-05-06 last obs.
|title = JPL Small-Body Database Browser: 1153 Wallenbergia (1924 SL)
|url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001153
|publisher = Jet Propulsion Laboratory
|accessdate = 8 September 2017}}</ref>

<ref name="springer">{{cite book
|title = Dictionary of Minor Planet Names – (1153) Wallenbergia
|last = Schmadel | first = Lutz D.
|publisher = Springer Berlin Heidelberg
|page = 97
|date = 2007
|url = https://link.springer.com/referenceworkentry/10.1007/978-3-540-29925-7_1154
|isbn = 978-3-540-00238-3
|accessdate = 8 September 2017}}</ref>

<ref name="MPC-object">{{cite web
|title = 1153 Wallenbergia (1924 SL)
|work = Minor Planet Center
|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1153
|accessdate = 8 September 2017}}</ref>

<ref name="lcdb">{{cite web
|title = LCDB Data for (1153) Wallenbergia
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1153%7CWallenbergia
|accessdate = 8 September 2017}}</ref>

<ref name="Masiero-2012">{{cite journal
|display-authors = 6
|first1 = Joseph R. |last1 = Masiero
|first2 = A. K. |last2 = Mainzer
|first3 = T. |last3 = Grav
|first4 = J. M. |last4 = Bauer
|first5 = R. M. |last5 = Cutri
|first6 = C. |last6 = Nugent
|first7 = M. S. |last7 = Cabrera
|date = November 2012
|title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
|journal = The Astrophysical Journal Letters
|volume = 759
|issue = 1
|page = 5
|bibcode = 2012ApJ...759L...8M
|doi = 10.1088/2041-8205/759/1/L8
|arxiv = 1209.5794
|access-date= 8 September 2017}}</ref>

<ref name="Nugent-2016">{{cite journal
|display-authors = 6
|first1 = C. R. |last1 = Nugent
|first2 = A. |last2 = Mainzer
|first3 = J. |last3 = Bauer
|first4 = R. M. |last4 = Cutri
|first5 = E. A. |last5 = Kramer
|first6 = T. |last6 = Grav
|first7 = J. |last7 = Masiero
|first8 = S. |last8 = Sonnett
|first9 = E. L. |last9 = Wright
|date = September 2016
|title = NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016AJ....152...63N
|journal = The Astronomical Journal
|volume = 152
|issue = 3
|page = 12
|bibcode = 2016AJ....152...63N
|doi = 10.3847/0004-6256/152/3/63
|arxiv = 1606.08923
|access-date= 8 September 2017}}</ref>

<ref name="Wisniewski-1997">{{Cite journal
|first1 = W. Z. |last1 = Wisniewski
|first2 = T. M. |last2 = Michalowski
|first3 = A. W. |last3 = Harris
|first4 = R. S. |last4 = McMillan
|date = March 1995
|title = Photoelectric Observations of 125 Asteroids
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1995LPI....26.1511W
|journal = Abstracts of the Lunar and Planetary Science Conference
|bibcode = 1995LPI....26.1511W
|access-date= 8 September 2017}}</ref>

<ref name="Chang-2015">{{cite journal
|display-authors = 6
|first1 = Chan-Kao |last1 = Chang
|first2 = Wing-Huen |last2 = Ip
|first3 = Hsing-Wen |last3 = Lin
|first4 = Yu-Chi |last4 = Cheng
|first5 = Chow-Choong |last5 = Ngeow
|first6 = Ting-Chang |last6 = Yang
|first7 = Adam |last7 = Waszczak
|first8 = Shrinivas R. |last8 = Kulkarni
|first9 = David |last9 = Levitan
|first10 = Branimir |last10 = Sesar
|first11 = Russ |last11 = Laher
|first12 = Jason |last12 = Surace
|first13 = Thomas. A. |last13 = Prince
|date = August 2015
|title = Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJS..219...27C
|journal = The Astrophysical Journal Supplement Series
|volume = 219
|issue = 2
|page = 19
|bibcode = 2015ApJS..219...27C
|doi = 10.1088/0067-0049/219/2/27
|arxiv = 1506.08493
|access-date= 8 September 2017}}</ref>

<ref name="Waszczak-2015">{{cite journal
|display-authors = 6
|first1 = Adam |last1 = Waszczak
|first2 = Chan-Kao |last2 = Chang
|first3 = Eran O. |last3 = Ofek
|first4 = Russ |last4 = Laher
|first5 = Frank |last5 = Masci
|first6 = David |last6 = Levitan
|first7 = Jason |last7 = Surace
|first8 = Yu-Chi |last8 = Cheng
|first9 = Wing-Huen |last9 = Ip
|first10 = Daisuke |last10 = Kinoshita
|first11 = George |last11 = Helou
|first12 = Thomas A. |last12 = Prince
|first13 = Shrinivas |last13 = Kulkarni
|date = September 2015
|title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W
|journal = The Astronomical Journal
|volume = 150
|issue = 3
|page = 35
|bibcode = 2015AJ....150...75W
|doi = 10.1088/0004-6256/150/3/75
|arxiv = 1504.04041
|access-date= 8 September 2017}}</ref>

<ref name="Pravec-2012b">{{Cite journal
|first1 = Petr |last1 = Pravec
|first2 = Alan W. |last2 = Harris
|first3 = Peter |last3 = Kusnirák
|first4 = Adrián |last4 = Galád
|first5 = Kamil |last5 = Hornoch
|date = September 2012
|title = Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012Icar..221..365P
|journal = Icarus
|volume = 221
|issue = 1
|pages = 365–387
|bibcode = 2012Icar..221..365P
|doi = 10.1016/j.icarus.2012.07.026
|access-date= 8 September 2017}}</ref>

<ref name="Veres-2015">{{cite journal
|display-authors = 6
|first1 = Peter |last1 = Veres
|first2 = Robert |last2 = Jedicke
|first3 = Alan |last3 = Fitzsimmons
|first4 = Larry |last4 = Denneau
|first5 = Mikael |last5 = Granvik
|first6 = Bryce |last6 = Bolin
|first7 = Serge |last7 = Chastel
|first8 = Richard J. |last8 = Wainscoat
|first9 = William S. |last9 = Burgett
|first10 = Kenneth C. |last10 = Chambers
|first11 = Heather |last11 = Flewelling
|first12 = Nick |last12 = Kaiser
|first13 = Eugen A. |last13 = Magnier
|first14 = Jeff S. |last14 = Morgan
|first15 = Paul A. |last15 = Price
|first16 = John L. |last16 = Tonry
|first17 = Christopher |last17 = Waters
|date = November 2015
|title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
|journal = Icarus
|volume = 261
|pages = 34–47
|bibcode = 2015Icar..261...34V
|doi = 10.1016/j.icarus.2015.08.007
|arxiv = 1506.00762
|access-date= 8 September 2017}}</ref>

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

== External links ==
* [https://archive.org/details/theoriederlinea00guldgoog Theorie der linearen Differenzengleichungen], by Georg Wallenberg , Alf Guldberg
* [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html 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] – Observatoire de Genève, Raoul Behrend
* [http://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
* {{JPL small body}}
* {{JPL small body}}


{{Minor planets navigator|1152 Pawona|number=1153|1154 Astronomia}}
{{Minor planets navigator |1152 Pawona |number=1153 |1154 Astronomia}}
{{Small Solar System bodies}}
{{Small Solar System bodies}}


{{DEFAULTSORT:Wallenbergia}}
{{DEFAULTSORT:Wallenbergia}}
[[Category:Main-belt asteroids|001153]]
[[Category:Flora asteroids|001153]]
[[Category:Numbered minor planets|001153]]
[[Category:Numbered minor planets|001153]]
[[Category:Discoveries by Sergei Belyavsky]]
[[Category:Minor planets named for people]]
[[Category:Minor planets named for people]]
[[Category:Named minor planets]]
[[Category:Named minor planets]]
[[Category:Discoveries by Sergei Belyavsky]]
[[Category:Astronomical objects discovered in 1924|19240905]]
[[Category:Astronomical objects discovered in 1924|19240905]]


{{beltasteroid-stub}}

Revision as of 00:38, 8 September 2017

1153 Wallenbergia
Discovery [1]
Discovered byS. Belyavskyj
Discovery siteSimeiz Obs.
Discovery date5 September 1924
Designations
(1153) Wallenbergia
Named after
Georg Wallenberg [2][a]
(German mathematician)
1924 SL · 1930 HH
main-belt · (inner) · Flora [3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.02 yr (31,784 days)
Aphelion2.5489 AU
Perihelion1.8428 AU
2.1958 AU
Eccentricity0.1608
3.25 yr (1,189 days)
237.52°
0° 18m 10.44s / day
Inclination3.3345°
280.54°
28.766°
Physical characteristics
Dimensions8.02±1.81 km[4]
8.037±0.357 km[5]
9.36 km (derived)[3]
4.096±0.002 h[6]
4.116±0.0055 h[7]
4.12±0.070 h[8]
0.24 (assumed)[3]
0.37±0.14[4]
0.433±0.091[5]
S [3][9]
11.985±0.002 (R)[7] · 12.00[5] · 12.040±0.100 (R)[8] · 12.1[1] · 12.28[4] · 12.31±0.08[3][6][10] · 12.49±0.22[9]

1153 Wallenbergia, provisional designation 1924 SL, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 5 September 1924, by Soviet astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula.[11] The asteroid was named after German mathematician Georg Wallenberg.[2]

Orbit and classification

Wallenbergia is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the main-belt.[3] It orbits the Sun in the inner main-belt at a distance of 1.8–2.5 AU once every 3 years and 3 months (1,189 days). Its orbit has an eccentricity of 0.16 and an inclination of 3° with respect to the ecliptic.[1]

The body's observation arc begins with its identification as 1930 HH at Johannesburg Observatory in April 1930, almost six years after its official discovery observation at Simeiz.[11]

Physical characteristics

Wallenbergia has been characterized as a stony S-type asteroid by PanSTARRS photometric survey.[9]

Rotation period

In September 1989, the first rotational lightcurve of Wallenbergia was obtained from photometric observations by Polish astronomer Wiesław Z. Wiśniewski at University of Arizona. Lightcurve analysis gave a well-defined rotation period of 4.096 hours with a brightness amplitude of 0.33 magnitude (U=3).[6] Observations in the R-band at the Palomar Transient Factory in 2012, gave a period of 4.116 and 4.12 hours with an amplitude of 0.25 and 0.23 magnitude, respectively (U=2/2).[7][8]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Wallenbergia measures 8.02 and 8.037 kilometers in diameter and its surface has an albedo of 0.37 and 0.433, respectively.[4][5]

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from 8 Flora, the parent body of the Flora family – and derives a diameter of 9.36 kilometers based on an absolute magnitude of 12.31.[3]

Naming

This minor planet was named after German mathematician Georg Wallenberg (1864–1924). The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 107).[2][a]

Notes

  1. ^ a b Wallenberg's middle name is likely "Jakob", not "James" as given in the Dictionary of Minor Planet Names

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1153 Wallenbergia (1924 SL)" (2017-05-06 last obs.). Jet Propulsion Laboratory. Retrieved 8 September 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (1153) Wallenbergia. Springer Berlin Heidelberg. p. 97. ISBN 978-3-540-00238-3. Retrieved 8 September 2017.
  3. ^ a b c d e f g "LCDB Data for (1153) Wallenbergia". Asteroid Lightcurve Database (LCDB). Retrieved 8 September 2017.
  4. ^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63. Retrieved 8 September 2017.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  5. ^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved 8 September 2017.
  6. ^ a b c Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids". Abstracts of the Lunar and Planetary Science Conference. Bibcode:1995LPI....26.1511W. Retrieved 8 September 2017.
  7. ^ a b c Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 8 September 2017.
  8. ^ a b c Chang, Chan-Kao; Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015). "Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory". The Astrophysical Journal Supplement Series. 219 (2): 19. arXiv:1506.08493. Bibcode:2015ApJS..219...27C. doi:10.1088/0067-0049/219/2/27. Retrieved 8 September 2017.
  9. ^ a b c Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 8 September 2017.
  10. ^ Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. Retrieved 8 September 2017.
  11. ^ a b "1153 Wallenbergia (1924 SL)". Minor Planet Center. Retrieved 8 September 2017.

External links

Retrieved from "https://en.wikipedia.org/w/index.php?title=1153_Wallenbergia&oldid=799485172"