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1796 Riga

1796 Riga, provisional designation 1966 KB, is a dark asteroid from the outer region of the asteroid belt, approximately 70 kilometers in diameter. It was discovered on 16 May 1966, by Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[15] It is named after the Latvian capital Riga.[2]

1796 Riga
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date16 May 1966
Designations
(1796) Riga
Named after
Riga (capital city)[2]
1966 KB · 1935 GE
1941 FC1 · 1947 GA
1950 TF2 · 1953 GW
1960 JA · A907 TG
A907 UD
main-belt · (outer)[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.06 yr (24,129 days)
Aphelion3.5474 AU
Perihelion3.1668 AU
3.3571 AU
Eccentricity0.0567
6.15 yr (2,247 days)
142.11°
0° 9m 36.72s / day
Inclination22.585°
186.73°
25.620°
Physical characteristics
Dimensions66.2±6.6 km[3]
68.089±1.037 km[4]
68.167±0.298 km[5]
71±7 km[6]
73.83±1.8 km[7]
85.79±1.57 km[8]
10.608±0.002 h[9][a]
11.0±0.01 h[10]
16 h[11]
22.226±0.001 h[12]
0.028±0.001[8]
0.0376±0.002[7]
0.04±0.01[6]
0.044±0.005[5]
0.0442±0.0082[4]
0.05±0.01[3]
XFCU (Tholen)[1]
Cb (SMASS)[1]
P[4] · C[13][14]
B–V = 0.676[1]
U–B = 0.289[1]
9.59±0.40[14] · 9.84 (IRAS:12)[1][7] · 9.84[3][4][6][8][13]

Orbit and classification edit

The asteroid orbits the Sun in the outer main-belt at a distance of 3.2–3.5 AU once every 6 years and 2 months (2,247 days). Its orbit has an eccentricity of 0.06 and an inclination of 23° with respect to the ecliptic.[1] The body was first identified as "1907 TG" at the U.S Taunton Observatory (803) in 1907, and its first used precovery was taken at the Goethe Link Observatory in 1953, extending the asteroid's observation arc by 13 years prior to its official discovery observation.[15] It is a member of the Cybele group of asteroids.[16]

Spectral type edit

The carbonaceous C-type asteroid is also classified as a very dark and featureless reddish P-type body by the NEOWISE survey of the Wide-field Infrared Survey Explorer (WISE).[4][13][14] In the Tholen and SMASS taxonomy, it has a XFCU and Cb subtype, respectively.[1]

Diameter and albedo edit

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and NASA's WISE/NEOWISE mission, the asteroid measures between 66.2 and 85.7 kilometers in diameter and its surface has an albedo between 0.028 and 0.05.[3][4][5][6][7][8] The Collaborative Asteroid Lightcurve Link (CALL) agrees with the results obtained by IRAS, adopting a diameter of 73.83 kilometers with an albedo of 0.0376, based on an absolute magnitude of 9.84.[13]

Rotation period edit

Several rotational lightcurve for this asteroid were obtained from photometric observations since 1997. They gave a variety of rotation periods from 10.608 to 22.226 hours with inconsistent brightness variations in the range of 0.05 to 0.40 magnitude (U=2/2-/n.a./2).[9][10][11][12][a] CALL adopts the results of the most observations made by astronomer Julian Oey at the Australian Blue Mountains Observatory (Q68) in March 2014, which gave a period of 22.226±0.001 hours and an amplitude of 0.40±0.05 magnitude (U=2).[12][13]

Naming edit

The minor planet was named after Riga, the capital of Latvia and location of the Astronomical Observatory of the University of Latvia. The name was proposed by Matiss A. Dirikis, who was a member of the observatory at the Latvian State University, and after whom the asteroid 1805 Dirikis is named.[2] The official naming citation was published by the Minor Planet Center on 25 September 1971 (M.P.C. 3185).[17]

Notes edit

  1. ^ a b Lightcurve plot of 1796 Riga, Palmer Divide Observatory, by B. D. Warner (2003), with a rotation period 10.608±0.002 hours and a brightness amplitude of 0.14±0.02 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)

References edit

  1. ^ a b c d e f g h i j "JPL Small-Body Database Browser: 1796 Riga (1966 KB)" (2016-11-04 last obs.). Jet Propulsion Laboratory. Retrieved 1 July 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1796) Riga". Dictionary of Minor Planet Names – (1796) Riga. Springer Berlin Heidelberg. p. 144. doi:10.1007/978-3-540-29925-7_1797. ISBN 978-3-540-00238-3.
  3. ^ a b c d Alí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics. 591: 11. Bibcode:2016A&A...591A..14A. doi:10.1051/0004-6361/201527660. hdl:11336/63614. Retrieved 10 August 2016.
  4. ^ a b c d e f Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90.
  5. ^ 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. Retrieved 29 October 2016.
  6. ^ a b c d Alí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013). "Physical properties of B-type asteroids from WISE data". Astronomy and Astrophysics. 554: 16. arXiv:1303.5487. Bibcode:2013A&A...554A..71A. doi:10.1051/0004-6361/201220680. Retrieved 29 October 2016.
  7. ^ 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 – IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 17 October 2019.
  8. ^ 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)
  9. ^ a b Warner, Brian D. (April 2011). "Upon Further Review: VI. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory". The Minor Planet Bulletin. 38 (2): 96–101. Bibcode:2011MPBu...38...96W. ISSN 1052-8091. Retrieved 17 November 2015.
  10. ^ a b Warner, Brian D. (March 2004). "Rotation rates for asteroids 875, 926, 1679, 1796, 3915, 4209, and 34817". The Minor Planet Bulletin. 31 (1): 19–22. Bibcode:2004MPBu...31...19W. ISSN 1052-8091. Retrieved 17 November 2015.
  11. ^ a b Chiorny, V. G.; Shevchenko, V. G.; Krugly, Yu. N.; Velichko, F. P.; Gaftonyuk, N. M. (May 2007). "Photometry of asteroids: Lightcurves of 24 asteroids obtained in 1993 2005". Planetary and Space Science. 55 (7–8): 986–997. Bibcode:2007P&SS...55..986C. doi:10.1016/j.pss.2007.01.001. Retrieved 17 November 2015.
  12. ^ a b c Oey, Julian (January 2016). "Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2014". The Minor Planet Bulletin. 43 (1): 45–51. Bibcode:2016MPBu...43...45O. ISSN 1052-8091. Retrieved 29 October 2016.
  13. ^ a b c d e "LCDB Data for (1796) Riga". Asteroid Lightcurve Database (LCDB). Retrieved 29 October 2016.
  14. ^ 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 29 October 2016.
  15. ^ a b "1796 Riga (1966 KB)". Minor Planet Center. Retrieved 29 October 2016.
  16. ^ De Prá, M. N.; et al. (September 2018), "PRIMASS visits Hilda and Cybele groups", Icarus, 311: 35–51, arXiv:1711.02071, Bibcode:2018Icar..311...35D, doi:10.1016/j.icarus.2017.11.012.
  17. ^ Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN 978-3-642-01964-7.

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
  • 1796 Riga at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 1796 Riga at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

1796, riga, provisional, designation, 1966, dark, asteroid, from, outer, region, asteroid, belt, approximately, kilometers, diameter, discovered, 1966, russian, astronomer, nikolai, chernykh, crimean, astrophysical, observatory, nauchnyj, crimean, peninsula, n. 1796 Riga provisional designation 1966 KB is a dark asteroid from the outer region of the asteroid belt approximately 70 kilometers in diameter It was discovered on 16 May 1966 by Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula 15 It is named after the Latvian capital Riga 2 1796 RigaDiscovery 1 Discovered byN ChernykhDiscovery siteCrimean Astrophysical Obs Discovery date16 May 1966DesignationsMPC designation 1796 RigaNamed afterRiga capital city 2 Alternative designations1966 KB 1935 GE1941 FC1 1947 GA1950 TF2 1953 GW1960 JA A907 TGA907 UDMinor planet categorymain belt outer 1 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc66 06 yr 24 129 days Aphelion3 5474 AUPerihelion3 1668 AUSemi major axis3 3571 AUEccentricity0 0567Orbital period sidereal 6 15 yr 2 247 days Mean anomaly142 11 Mean motion0 9m 36 72s dayInclination22 585 Longitude of ascending node186 73 Argument of perihelion25 620 Physical characteristicsDimensions66 2 6 6 km 3 68 089 1 037 km 4 68 167 0 298 km 5 71 7 km 6 73 83 1 8 km 7 85 79 1 57 km 8 Synodic rotation period10 608 0 002 h 9 a 11 0 0 01 h 10 16 h 11 22 226 0 001 h 12 Geometric albedo0 028 0 001 8 0 0376 0 002 7 0 04 0 01 6 0 044 0 005 5 0 0442 0 0082 4 0 05 0 01 3 Spectral typeXFCU Tholen 1 Cb SMASS 1 P 4 C 13 14 B V 0 676 1 U B 0 289 1 Absolute magnitude H 9 59 0 40 14 9 84 IRAS 12 1 7 9 84 3 4 6 8 13 Contents 1 Orbit and classification 2 Spectral type 3 Diameter and albedo 4 Rotation period 5 Naming 6 Notes 7 References 8 External linksOrbit and classification editThe asteroid orbits the Sun in the outer main belt at a distance of 3 2 3 5 AU once every 6 years and 2 months 2 247 days Its orbit has an eccentricity of 0 06 and an inclination of 23 with respect to the ecliptic 1 The body was first identified as 1907 TG at the U S Taunton Observatory 803 in 1907 and its first used precovery was taken at the Goethe Link Observatory in 1953 extending the asteroid s observation arc by 13 years prior to its official discovery observation 15 It is a member of the Cybele group of asteroids 16 Spectral type editThe carbonaceous C type asteroid is also classified as a very dark and featureless reddish P type body by the NEOWISE survey of the Wide field Infrared Survey Explorer WISE 4 13 14 In the Tholen and SMASS taxonomy it has a XFCU and Cb subtype respectively 1 Diameter and albedo editAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS the Japanese Akari satellite and NASA s WISE NEOWISE mission the asteroid measures between 66 2 and 85 7 kilometers in diameter and its surface has an albedo between 0 028 and 0 05 3 4 5 6 7 8 The Collaborative Asteroid Lightcurve Link CALL agrees with the results obtained by IRAS adopting a diameter of 73 83 kilometers with an albedo of 0 0376 based on an absolute magnitude of 9 84 13 Rotation period editSeveral rotational lightcurve for this asteroid were obtained from photometric observations since 1997 They gave a variety of rotation periods from 10 608 to 22 226 hours with inconsistent brightness variations in the range of 0 05 to 0 40 magnitude U 2 2 n a 2 9 10 11 12 a CALL adopts the results of the most observations made by astronomer Julian Oey at the Australian Blue Mountains Observatory Q68 in March 2014 which gave a period of 22 226 0 001 hours and an amplitude of 0 40 0 05 magnitude U 2 12 13 Naming editThe minor planet was named after Riga the capital of Latvia and location of the Astronomical Observatory of the University of Latvia The name was proposed by Matiss A Dirikis who was a member of the observatory at the Latvian State University and after whom the asteroid 1805 Dirikis is named 2 The official naming citation was published by the Minor Planet Center on 25 September 1971 M P C 3185 17 Notes edit a b Lightcurve plot of 1796 Riga Palmer Divide Observatory by B D Warner 2003 with a rotation period 10 608 0 002 hours and a brightness amplitude of 0 14 0 02 mag Summary figures at Collaborative Asteroid Lightcurve Link CALL References edit a b c d e f g h i j JPL Small Body Database Browser 1796 Riga 1966 KB 2016 11 04 last obs Jet Propulsion Laboratory Retrieved 1 July 2017 a b c Schmadel Lutz D 2007 1796 Riga Dictionary of Minor Planet Names 1796 Riga Springer Berlin Heidelberg p 144 doi 10 1007 978 3 540 29925 7 1797 ISBN 978 3 540 00238 3 a b c d Ali Lagoa V Licandro J Gil Hutton R Can ada Assandri M Delbo M et al June 2016 Differences between the Pallas collisional family and similarly sized B type asteroids Astronomy and Astrophysics 591 11 Bibcode 2016A amp A 591A 14A doi 10 1051 0004 6361 201527660 hdl 11336 63614 Retrieved 10 August 2016 a b c d e f Mainzer A Grav T Masiero J Hand E Bauer J Tholen D et al November 2011 NEOWISE Studies of Spectrophotometrically Classified Asteroids Preliminary Results The Astrophysical Journal 741 2 25 arXiv 1109 6407 Bibcode 2011ApJ 741 90M doi 10 1088 0004 637X 741 2 90 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 Retrieved 29 October 2016 a b c d Ali Lagoa V de Leon J Licandro J Delbo M Campins H Pinilla Alonso N et al June 2013 Physical properties of B type asteroids from WISE data Astronomy and Astrophysics 554 16 arXiv 1303 5487 Bibcode 2013A amp A 554A 71A doi 10 1051 0004 6361 201220680 Retrieved 29 October 2016 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 IRAS A FPA 3 RDR IMPS V6 0 Bibcode 2004PDSS 12 T Retrieved 17 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 Warner Brian D April 2011 Upon Further Review VI An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory The Minor Planet Bulletin 38 2 96 101 Bibcode 2011MPBu 38 96W ISSN 1052 8091 Retrieved 17 November 2015 a b Warner Brian D March 2004 Rotation rates for asteroids 875 926 1679 1796 3915 4209 and 34817 The Minor Planet Bulletin 31 1 19 22 Bibcode 2004MPBu 31 19W ISSN 1052 8091 Retrieved 17 November 2015 a b Chiorny V G Shevchenko V G Krugly Yu N Velichko F P Gaftonyuk N M May 2007 Photometry of asteroids Lightcurves of 24 asteroids obtained in 1993 2005 Planetary and Space Science 55 7 8 986 997 Bibcode 2007P amp SS 55 986C doi 10 1016 j pss 2007 01 001 Retrieved 17 November 2015 a b c Oey Julian January 2016 Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2014 The Minor Planet Bulletin 43 1 45 51 Bibcode 2016MPBu 43 45O ISSN 1052 8091 Retrieved 29 October 2016 a b c d e LCDB Data for 1796 Riga Asteroid Lightcurve Database LCDB Retrieved 29 October 2016 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 29 October 2016 a b 1796 Riga 1966 KB Minor Planet Center Retrieved 29 October 2016 De Pra M N et al September 2018 PRIMASS visits Hilda and Cybele groups Icarus 311 35 51 arXiv 1711 02071 Bibcode 2018Icar 311 35D doi 10 1016 j icarus 2017 11 012 Schmadel Lutz D Appendix Publication Dates of the MPCs Dictionary of Minor Planet Names Addendum to Fifth Edition 2006 2008 Springer Berlin Heidelberg p 221 doi 10 1007 978 3 642 01965 4 ISBN 978 3 642 01964 7 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 1796 Riga at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 1796 Riga 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 1796 Riga amp oldid 1195831609, wikipedia, wiki, book, books, library,

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