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1144 Oda

1144 Oda, provisional designation 1930 BJ, is a dark Hildian asteroid from the outermost regions of the asteroid belt, approximately 57 kilometers in diameter. It was discovered on 28 January 1930, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory.[10] The asteroid's name is a German female name, not related to the discoverer's contemporaries.[2]

1144 Oda
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date28 January 1930
Designations
(1144) Oda
Named after
A girl's name picked from a
popular German calendar[2]
1930 BJ · 1959 CJ
1967 EV
main-belt · (outer)
Hilda[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.27 yr (31,875 days)
Aphelion4.1018 AU
Perihelion3.3959 AU
3.7489 AU
Eccentricity0.0942
7.26 yr (2,651 days)
131.28°
0° 8m 8.88s / day
Inclination9.7423°
156.73°
220.87°
Physical characteristics
Dimensions56.347±0.194 km[4]
57.59±2.2 km[5]
57.65 km (derived)[3]
64.21±0.96 km[6]
14.4 h (dated)[7]
44.023±0.2530 h[8]
0.043±0.001[6]
0.0533±0.004[5]
0.0583 (derived)[3]
0.061±0.014[4]
Tholen = D[1][3] · X[9]
B–V = 0.706[1]
U–B = 0.249[1]
9.794±0.002 (R)[8] · 9.9[3] · 10.00[1][5][6] · 10.05±0.54[9]

Orbit and classification Edit

Oda belongs to the dynamical Hilda group which is located in the outermost part of the main belt.[3] Asteroids in this group have semi-major axis between 3.7 and 4.2 AU and stay in a 3:2 resonance with the gas giant Jupiter. Oda, however, is a non-family background asteroid, i.e. not a member of the collisional Hilda family (001).[11]

It orbits the Sun in the outer main belt at a distance of 3.4–4.1 AU once every 7 years and 3 months (2,651 days). Its orbit has an eccentricity of 0.09 and an inclination of 10° with respect to the ecliptic.[1] The body's observation arc begins at Heidelberg, two months after its official discovery observation.[10]

Physical characteristics Edit

In the Tholen classification, Oda is a dark and reddish D-type asteroid.[1] It has also been characterized as an X-type by PanSTARRS photometric survey.[9]

Rotation period Edit

In May 2011, a rotational lightcurve of Oda was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 44.023 hours with a brightness variation of 0.41 magnitude (U=2).[8] A previously measured period of 14.4 is now considered incorrect (U=1).[7]

While not being a slow rotator, which have periods above 100 hours, Oda's spin rate is significantly longer than that of most other asteroids that have periods shorter than 20 hours.

Diameter and albedo Edit

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Oda measures between 56.347 and 64.21 kilometers in diameter and its surface has an albedo between 0.043 and 0.061.[4][5][6]

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0583 and a diameter of 57.65 kilometers based on an absolute magnitude of 9.9.[3]

Naming Edit

This minor planet was named after a girl's name picked from the German popular calendar Der Lahrer hinkende Bote (de).

As with 913 Otila, Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries. The author of the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]

References Edit

  1. ^ a b c d e f g h "JPL Small-Body Database Browser: 1144 Oda (1930 BJ)" (2017-05-06 last obs.). Jet Propulsion Laboratory. Retrieved 9 September 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1144) Oda". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 97. doi:10.1007/978-3-540-29925-7_1145. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f g "LCDB Data for (1144) Oda". Asteroid Lightcurve Database (LCDB). Retrieved 9 September 2017.
  4. ^ a b c Grav, T.; Mainzer, A. K.; Bauer, J.; Masiero, J.; Spahr, T.; McMillan, R. S.; et al. (January 2012). "WISE/NEOWISE Observations of the Hilda Population: Preliminary Results". The Astrophysical Journal. 744 (2): 15. arXiv:1110.0283. Bibcode:2012ApJ...744..197G. doi:10.1088/0004-637X/744/2/197. S2CID 44000310. Retrieved 9 September 2017.
  5. ^ a b c d 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 22 October 2019.
  6. ^ a b c d 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. (online, AcuA catalog p. 153)
  7. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1144) Oda". Geneva Observatory. Retrieved 9 September 2017.
  8. ^ 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. S2CID 8342929. Retrieved 9 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. S2CID 53493339.
  10. ^ a b "1144 Oda (1930 BJ)". Minor Planet Center. Retrieved 9 September 2017.
  11. ^ "Asteroid 1144 Oda – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 28 October 2019.

External links Edit

  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • 1144 Oda at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 1144 Oda at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

1144, provisional, designation, 1930, dark, hildian, asteroid, from, outermost, regions, asteroid, belt, approximately, kilometers, diameter, discovered, january, 1930, german, astronomer, karl, reinmuth, heidelberg, königstuhl, state, observatory, asteroid, n. 1144 Oda provisional designation 1930 BJ is a dark Hildian asteroid from the outermost regions of the asteroid belt approximately 57 kilometers in diameter It was discovered on 28 January 1930 by German astronomer Karl Reinmuth at the Heidelberg Konigstuhl State Observatory 10 The asteroid s name is a German female name not related to the discoverer s contemporaries 2 1144 OdaDiscovery 1 Discovered byK ReinmuthDiscovery siteHeidelberg Obs Discovery date28 January 1930DesignationsMPC designation 1144 OdaNamed afterA girl s name picked from apopular German calendar 2 Alternative designations1930 BJ 1959 CJ1967 EVMinor planet categorymain belt outer Hilda 3 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc87 27 yr 31 875 days Aphelion4 1018 AUPerihelion3 3959 AUSemi major axis3 7489 AUEccentricity0 0942Orbital period sidereal 7 26 yr 2 651 days Mean anomaly131 28 Mean motion0 8m 8 88s dayInclination9 7423 Longitude of ascending node156 73 Argument of perihelion220 87 Physical characteristicsDimensions56 347 0 194 km 4 57 59 2 2 km 5 57 65 km derived 3 64 21 0 96 km 6 Synodic rotation period14 4 h dated 7 44 023 0 2530 h 8 Geometric albedo0 043 0 001 6 0 0533 0 004 5 0 0583 derived 3 0 061 0 014 4 Spectral typeTholen D 1 3 X 9 B V 0 706 1 U B 0 249 1 Absolute magnitude H 9 794 0 002 R 8 9 9 3 10 00 1 5 6 10 05 0 54 9 Contents 1 Orbit and classification 2 Physical characteristics 2 1 Rotation period 2 2 Diameter and albedo 3 Naming 4 References 5 External linksOrbit and classification EditOda belongs to the dynamical Hilda group which is located in the outermost part of the main belt 3 Asteroids in this group have semi major axis between 3 7 and 4 2 AU and stay in a 3 2 resonance with the gas giant Jupiter Oda however is a non family background asteroid i e not a member of the collisional Hilda family 001 11 It orbits the Sun in the outer main belt at a distance of 3 4 4 1 AU once every 7 years and 3 months 2 651 days Its orbit has an eccentricity of 0 09 and an inclination of 10 with respect to the ecliptic 1 The body s observation arc begins at Heidelberg two months after its official discovery observation 10 Physical characteristics EditIn the Tholen classification Oda is a dark and reddish D type asteroid 1 It has also been characterized as an X type by PanSTARRS photometric survey 9 Rotation period Edit In May 2011 a rotational lightcurve of Oda was obtained from photometric observations in the R band by astronomers at the Palomar Transient Factory in California Lightcurve analysis gave a rotation period of 44 023 hours with a brightness variation of 0 41 magnitude U 2 8 A previously measured period of 14 4 is now considered incorrect U 1 7 While not being a slow rotator which have periods above 100 hours Oda s spin rate is significantly longer than that of most other asteroids that have periods shorter than 20 hours Diameter and albedo Edit According to the surveys carried out by the Infrared Astronomical Satellite IRAS the Japanese Akari satellite and the NEOWISE mission of NASA s Wide field Infrared Survey Explorer Oda measures between 56 347 and 64 21 kilometers in diameter and its surface has an albedo between 0 043 and 0 061 4 5 6 The Collaborative Asteroid Lightcurve Link derives an albedo of 0 0583 and a diameter of 57 65 kilometers based on an absolute magnitude of 9 9 3 Naming EditThis minor planet was named after a girl s name picked from the German popular calendar Der Lahrer hinkende Bote de As with 913 Otila Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names These names are not related to the discoverer s contemporaries The author of the Dictionary of Minor Planet Names learned about Reinmuth s source of inspiration from private communications with Dutch astronomer Ingrid van Houten Groeneveld who worked as a young astronomer at Heidelberg 2 References Edit a b c d e f g h JPL Small Body Database Browser 1144 Oda 1930 BJ 2017 05 06 last obs Jet Propulsion Laboratory Retrieved 9 September 2017 a b c Schmadel Lutz D 2007 1144 Oda Dictionary of Minor Planet Names Springer Berlin Heidelberg p 97 doi 10 1007 978 3 540 29925 7 1145 ISBN 978 3 540 00238 3 a b c d e f g LCDB Data for 1144 Oda Asteroid Lightcurve Database LCDB Retrieved 9 September 2017 a b c Grav T Mainzer A K Bauer J Masiero J Spahr T McMillan R S et al January 2012 WISE NEOWISE Observations of the Hilda Population Preliminary Results The Astrophysical Journal 744 2 15 arXiv 1110 0283 Bibcode 2012ApJ 744 197G doi 10 1088 0004 637X 744 2 197 S2CID 44000310 Retrieved 9 September 2017 a b c d 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 22 October 2019 a b c d Usui Fumihiko Kuroda Daisuke Muller 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 online AcuA catalog p 153 a b Behrend Raoul Asteroids and comets rotation curves 1144 Oda Geneva Observatory Retrieved 9 September 2017 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 S2CID 8342929 Retrieved 9 September 2017 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 S2CID 53493339 a b 1144 Oda 1930 BJ Minor Planet Center Retrieved 9 September 2017 Asteroid 1144 Oda Proper Elements AstDyS 2 Asteroids Dynamic Site Retrieved 28 October 2019 External links EditAsteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 1144 Oda at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 1144 Oda at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 1144 Oda amp oldid 1173445010, wikipedia, wiki, book, books, library,

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