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5143 Heracles

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5143 Heracles
Discovery [1]
Discovered byC. Shoemaker
Discovery sitePalomar Obs.
Discovery date7 November 1991
Designations
(5143) Heracles
Pronunciation/ˈhɛrəkliːz/
Named after
Ἡρακλῆς Hēraklēs (Greek mythology)[2]
1991 VL · 1962 PG
Apollo · NEO [1][3]
AdjectivesHeraclean /hɛrəˈkliːən/[4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.58 yr (23,224 days)
Earliest precovery date30 November 1953
Aphelion3.2494 AU
Perihelion0.4174 AU
1.8334 AU
Eccentricity0.7723
2.48 yr (907 days)
93.744°
0° 23m 49.2s / day
Inclination9.0330°
309.52°
227.77°
Known satellites1[5][6][7] (0.6±0.3 km; orb. 17 h)
Earth MOID0.0584 AU · 22.8 LD
Physical characteristics
Dimensions3.26 km[8]
3.28±0.09 km[9]
3.41 km[10]
4.5±0.7 km[5]
4.83 km (taken)[11]
4.833 km[12]
4.843±0.378 km[13][14]
2.704±0.002 h[15][a]
2.7060±0.0002 h[16]
2.706±0.001 h[17]
2.7063 h[11]
2.7065±0.0005 h[5]
3.0149±0.0002 h[18]
5.990±0.0111 h[19]
0.1481[12]
0.20±0.05[5]
0.227±0.054[13][14]
0.38[10]
0.40±0.22[20]
0.412±0.030[9]
0.42[8]
SMASS = O [1]
Q [21] · C [22] · O [11]
V–R = 0.420±0.070[5]
13.786±0.004 (R)[19] · 13.8[13] · 14.0[1][8][9][22] · 14.10±0.04[5] · 14.27[11][23] · 14.27±0.09[12] · 14.52±0.02 (R)[16]

5143 Heracles (provisional designation 1991 VL) is a highly eccentric, rare-type asteroid and synchronous binary system, classified as near-Earth object of the Apollo group, approximately 4.8 kilometers in diameter. The asteroid was discovered on 7 November 1991, by American astronomer Carolyn Shoemaker at Palomar Observatory in California, United States.[3] It is named for the Greek divine hero Heracles.[2] It has an Earth minimum orbit intersection distance of 0.058 AU (8.7 million km) and is associated with the Beta Taurids daytime meteor shower.[24]

Classification and orbit

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Heracles orbits the Sun in the inner main-belt at a distance of 0.4–3.2 AU once every 2 years and 6 months (907 days). Its orbit has an eccentricity of 0.77 and an inclination of 9° with respect to the ecliptic.[1] The first precovery was taken at Palomar during the Digitized Sky Survey in 1953, extending the body's observation arc by 38 years prior to its official discovery observation.[3]

Due to its high eccentricity, Heracles is also a Mercury-grazer and a Mars-crosser. It has a minimum orbital intersection distance with Earth of 0.0584 AU (8,740,000 km) which corresponds to 22.8 lunar distances.[1]

Physical characteristics

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Spectral type

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In the SMASS taxonomy, Heracles is a rare O-type asteroid, which have spectra similar to those of stony chondritic meteorites of the L6 and LL6 type.[1] However, it has also been characterized as a carbonaceous C-type, as well as a stony Sk and Q-type asteroid.[21][22][25]

Lightcurves

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A large number of rotational lightcurves of Heracles were obtained from photometric observations between 2006 and 2016. Lightcurve data gives a rotation period between 2.7051 and 2.7065 hours with a brightness variation of 0.05 to 0.20 magnitude (U=3/3/3/3/3-).[5][11][15][16][a]

Diameters

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According to the surveys carried out by the Spitzer Space Telescope, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 3.26 and 4.843 kilometers in diameter, and its surface has an albedo between 0.20 and 0.24.[8][9][10][13] The Collaborative Asteroid Lightcurve Link adopts the results from Petr Pravec's revised WISE data, that is, an albedo of 0.1481 and a diameter of 4.83 kilometers with an absolute magnitude of 14.27.[11][12]

Binary system

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On 12 July 2012, it was announced that Heracles is an assumed synchronous binary asteroid with a minor-planet moon orbiting its primary in a retrograde motion approximately every 16 hours. The companion was discovered in December 2011, by a team of astronomers using radar observations from Arecibo Observatory in Puerto Rico, following months of intensive photometric lightcurve observations (see above). It was designated S/2011 (5143) 1.

The satellite received the nickname Omphale, after the wife of Heracles who birth to his children. A longer orbital period of 40–57 hours cannot be excluded, which would then no longer be a synchronous system. Estimated diameters for Heracles and its moon are 3.6±1.2 and 0.6±0.3 kilometer, respectively.[6][7][11]

Follow-up observations in 2016 confirmed an orbital period of 17 hours for the asteroid moon.[25]

Naming

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This minor planet was named after Heracles, the divine gatekeeper of Mount Olympus and one of the greatest heroes in Greek mythology, known for his strength and his Twelve Labors. Heracles is the son of Zeus and Alcmena, after whom the asteroids 5731 Zeus and 82 Alkmene were named. In the Roman adaptation, Heracles is known as Hercules.[2] The approved naming citation was published by the Minor Planet Center on 14 July 1992 (M.P.C. 20523).[26]

Notes

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  1. ^ a b Warner (2017c): lightcurve plot of (5143) Heracles, with a rotation period 2.704±0.002 hours and a brightness amplitude of 0.15 mag (Quality Code of 2; 133 points). Observations from 12 to 17 September 2016, at CS3-Palmer Divide Station. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^ a b c d e f g h "JPL Small-Body Database Browser: 5143 Heracles (1991 VL)" (2017-07-01 last obs.). Jet Propulsion Laboratory. Retrieved 4 July 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(5143) Heracles". Dictionary of Minor Planet Names – (5143) Heracles. Springer Berlin Heidelberg. p. 442. doi:10.1007/978-3-540-29925-7_4995. ISBN 978-3-540-00238-3.
  3. ^ a b c "5143 Heracles (1991 VL)". Minor Planet Center. Retrieved 14 March 2017.
  4. ^ "Heraclean". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  5. ^ a b c d e f g Pilcher, Frederick; Briggs, John W.; Franco, Lorenzo; Inasaridze, Raguli Ya.; Krugly, Yurij N.; Molotiv, Igor E.; et al. (July 2012). "Rotation Period Determination for 5143 Heracles". The Minor Planet Bulletin. 39 (3): 148–151. Bibcode:2012MPBu...39..148P. ISSN 1052-8091.
  6. ^ a b Taylor, P. A.; Nolan, M. C.; Howell, E. S. (July 2012). "(5143) Heracles". Central Bureau Electronic Telegrams. 3176 (3176): 1. Bibcode:2012CBET.3176....1T.
  7. ^ a b Lance A. M. Benner (18 November 2013). "Binary and Ternary near-Earth Asteroids detected by radar". NASA/JPL Asteroid Radar Research. Archived from the original on 8 June 2004. Retrieved 14 March 2017.
  8. ^ a b c d Trilling, D. E.; Mueller, M.; Hora, J. L.; Harris, A. W.; Bhattacharya, B.; Bottke, W. F.; et al. (September 2010). "ExploreNEOs. I. Description and First Results from the Warm Spitzer Near-Earth Object Survey" (PDF). The Astronomical Journal. 140 (3): 770–784. Bibcode:2010AJ....140..770T. doi:10.1088/0004-6256/140/3/770. S2CID 3006566.
  9. ^ 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)
  10. ^ a b c Harris, A. W.; Mommert, M.; Hora, J. L.; Mueller, M.; Trilling, D. E.; Bhattacharya, B.; et al. (March 2011). "ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey" (PDF). The Astronomical Journal. 141 (3): 10. Bibcode:2011AJ....141...75H. doi:10.1088/0004-6256/141/3/75. S2CID 14208889.
  11. ^ a b c d e f g "LCDB Data for (5143) Heracles". Asteroid Lightcurve Database (LCDB). Retrieved 14 March 2017.
  12. ^ a b c d 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.
  13. ^ a b c d 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. S2CID 118700974.
  14. ^ a b Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv:1109.6400. Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156. S2CID 239991.
  15. ^ a b Warner, Brian D. (January 2017). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2016 July-September". The Minor Planet Bulletin. 44 (1): 22–36. Bibcode:2017MPBu...44...22W. ISSN 1052-8091. PMC 7243971. PMID 32455389.
  16. ^ a b c Polishook, David (July 2012). "Lightcurves and Spin Periods of Near-Earth Asteroids, The Wise Observatory, 2005 - 2010". The Minor Planet Bulletin. 39 (3): 187–192. Bibcode:2012MPBu...39..187P. ISSN 1052-8091.
  17. ^ Linder, Tyler R.; Sampson, Ryan; Holmes, Robert (January 2013). "Astronomical Research Institute Photometric Results". The Minor Planet Bulletin. 40 (1): 4–6. Bibcode:2013MPBu...40....4L. ISSN 1052-8091.
  18. ^ Behrend, Raoul. "Asteroids and comets rotation curves – (5143) Heracles". Geneva Observatory. Retrieved 14 March 2017.
  19. ^ a b 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.
  20. ^ Thomas, C. A.; Trilling, D. E.; Emery, J. P.; Mueller, M.; Hora, J. L.; Benner, L. A. M.; et al. (September 2011). "ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population". The Astronomical Journal. 142 (3): 12. Bibcode:2011AJ....142...85T. doi:10.1088/0004-6256/142/3/85.
  21. ^ a b Thomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014). "Physical characterization of Warm Spitzer-observed near-Earth objects". Icarus. 228: 217–246. arXiv:1310.2000. Bibcode:2014Icar..228..217T. doi:10.1016/j.icarus.2013.10.004. S2CID 119278697.
  22. ^ a b c Carry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry". Icarus. 268: 340–354. arXiv:1601.02087. Bibcode:2016Icar..268..340C. doi:10.1016/j.icarus.2015.12.047. S2CID 119258489.
  23. ^ Pravec, Petr; Wolf, Marek; Sarounová, Lenka (November 1998). "Lightcurves of 26 Near-Earth Asteroids". Icarus. 136 (1): 124–153. Bibcode:1998Icar..136..124P. doi:10.1006/icar.1998.5993.
  24. ^ Babadzhanov, P. B. (2001). "Search for meteor showers associated with Near-Earth Asteroids". Astronomy and Astrophysics. 373 (1): 329–335. Bibcode:2001A&A...373..329B. doi:10.1051/0004-6361:20010583.
  25. ^ a b Taylor, P. A.; Howell, E. S.; Zambrano-Marin, L. F. (2017). "Radar and infrared Observations of Binary Near-Earth Asteroid (5143) Heracles" (PDF). Retrieved 14 March 2017. {{cite journal}}: Cite journal requires |journal= (help)
  26. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 14 March 2017.
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