3240 Laocoon is a carbonaceous Jupiter trojan from the Trojan camp , approximately 51 kilometers (32 miles) in diameter. It was discovered on 7 November 1978, by American astronomers Eleanor Helin and Schelte Bus at Palomar Observatory in California.[ 1] The D-type asteroid belongs to the 100 largest Jupiter trojans and has a rotation period of 11.3 hours.[ 9] It was named after Laocoön from Greek mythology.[ 3]
Classification and orbit
Laocoon resides in the Trojan camp of Jupiter's L5 Lagrangian point , which lies 60° behind the gas giant's orbit.[ 5] It is also a non-family asteroid of the Jovian background population .[ 6]
It orbits the Sun at a distance of 4.6–5.9 AU once every 11 years and 12 months (4,375 days; semi-major axis of 5.23 AU). Its orbit has an eccentricity of 0.13 and an inclination of 2° with respect to the ecliptic .[ 4] The asteroid was first observed as 1976 SL2 at Crimea–Nauchnij in September 1976, extending the body's observation arc by 2 years prior to its official discovery at Palomar.[ 1]
Physical characteristics
Laocoon has been characterized as a D-type asteroid by Pan-STARRS ' survey and in the SDSS -based taxonomy. It has a V–I color index of 0.88.[ 9] [ 10] [ 11]
Lightcurve
In April 1996, Laocoon was observed by Italian astronomer Stefano Mottola using the now decommissioned Bochum 0.61-metre Telescope at ESO's La Silla Observatory in Chile. The lightcurve gave a rotation period of 11.312± 0.024 hours with a brightness variation of 0.55± 0.02 in magnitude (U=2+ ).[ 9] [ 8]
Diameter and albedo
According to the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , the Jovian asteroid measures 51.7 kilometers in diameter and its surface has an albedo of 0.060,[ 7] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 50.8 kilometers with an absolute magnitude of 10.2.[ 9]
100+ largest Jupiter trojans
Naming
This minor planet was named after the Troyan priest Laocoön from Greek mythology . He and both his sons were killed by serpents sent by the gods because he tried to expose the Greek's deception of the Trojan Horse .[ 3] The official naming citation was published by the Minor Planet Center on 7 September 1987 (M.P.C. 12210 ).[ 13]
See also
References
^ a b c d e "3240 Laocoon (1978 VG6)" . Minor Planet Center . Retrieved 17 June 2018 .
^ Noah Webster (1884) A Practical Dictionary of the English Language
^ a b c Schmadel, Lutz D. (2007). "(3240) Laocoon". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 269. doi :10.1007/978-3-540-29925-7_3241 . ISBN 978-3-540-00238-3 .
^ a b c "JPL Small-Body Database Browser: 3240 Laocoon (1978 VG6)" (2018-05-19 last obs.). Jet Propulsion Laboratory . Retrieved 17 June 2018 .
^ a b "List of Jupiter Trojans" . Minor Planet Center . 1 June 2018. Retrieved 17 June 2018 .
^ a b "Asteroid (3240) Laocoon – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 17 June 2018 .
^ a b c d Grav, T.; Mainzer, A. K.; Bauer, J. M.; Masiero, J. R.; Nugent, C. R. (November 2012). "WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy" . The Astrophysical Journal . 759 (1): 10. arXiv :1209.1549 . Bibcode :2012ApJ...759...49G . doi :10.1088/0004-637X/759/1/49 . S2CID 119101711 . Retrieved 17 June 2018 . (online catalog )
^ a b Mottola, Stefano; Di Martino, Mario; Erikson, Anders; Gonano-Beurer, Maria; Carbognani, Albino; Carsenty, Uri; et al. (May 2011). "Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects" . The Astronomical Journal . 141 (5): 32. Bibcode :2011AJ....141..170M . doi :10.1088/0004-6256/141/5/170 .
^ a b c d e f g "LCDB Data for (3240) Laocoon" . Asteroid Lightcurve Database (LCDB). Retrieved 17 June 2018 .
^ a b 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 Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids" . Astronomy and Astrophysics . 510 : 12. Bibcode :2010A&A...510A..43C . doi :10.1051/0004-6361/200913322 . Retrieved 30 October 2019 . (PDS data set)
^ a b Chatelain, Joseph P.; Henry, Todd J.; French, Linda M.; Winters, Jennifer G.; Trilling, David E. (June 2016). "Photometric colors of the brightest members of the Jupiter L5 Trojan cloud" . Icarus . 271 : 158– 169. Bibcode :2016Icar..271..158C . doi :10.1016/j.icarus.2016.01.026 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 17 June 2018 .
External links