4341 Poseidon (prov. designation : 1987 KF ) is a rare-type asteroid classified as near-Earth object of the Apollo group , approximately 2.3 kilometers (1.4 miles) in diameter. It was discovered by American astronomer Carolyn Shoemaker at Palomar Observatory on 29 May 1987.[ 7] The asteroid was named after Poseidon from Greek mythology.[ 2]
Orbit and classification
Poseidon orbits the Sun at a distance of 0.6–3.1 AU once every 2 years and 6 months (908 days). Its orbit has an eccentricity of 0.68 and an inclination of 12° with respect to the ecliptic .[ 1]
As no precoveries were taken, the asteroid's observation arc begins with its discovery in 1987.[ 7] Poseidon may be associated with the Taurid Complex of meteor showers.[ 8] It has an Earth minimum orbital intersection distance of 0.1941 AU (29,000,000 km), which corresponds to 75.6 lunar distances .[ 1]
Naming
This minor planet was named for the "God of the Sea", Poseidon , one of the Twelve Olympians in Greek mythology . He was also referred to as "Earth-Shaker" due to his role in provoking earthquakes, which were then thought to be caused by ocean waves beating on the shore. He was the brother of Zeus (see 5731 Zeus ) , and an enemy of the Trojans in the Trojan War .[ 2] The naming citation was published by the Minor Planet Center on 30 January 1991 (M.P.C. 17656 ).[ 9]
Physical characteristics
In the SMASS classification , Poseidon is an O-type asteroid .[ 1]
Diameter and albedo
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.18 and derives a diameter of 2.32 kilometers with an absolute magnitude of 15.65.[ 3] As of 2017, no other estimates for its diameter and albedo have been published.[ 1] [ 3]
Lightcurves
In 1998, a rotational lightcurve of Poseidon was published from photometric observations made by Czech astronomer Petr Pravec at Ondřejov Observatory . It gave a period of 6.262 hours with a brightness variation of 0.08 magnitude (U=2 ).[ 4]
A second lightcurve was obtained during the Near-Earth Objects Follow-up Program which gave a concurring period of 6.2656 hours and an amplitude of 0.07 magnitude (U=2 ).[ 5] A low brightness variation typically indicates that the body has a nearly spheroidal shape.
References
^ a b c d e f g h "JPL Small-Body Database Browser: 4341 Poseidon (1987 KF)" (2017-06-15 last obs.). Jet Propulsion Laboratory . Retrieved 20 June 2017 .
^ a b c Schmadel, Lutz D. (2007). "(4341) Poseidon". Dictionary of Minor Planet Names – (4341) Poseidon . Springer Berlin Heidelberg . p. 372. doi :10.1007/978-3-540-29925-7_4293 . ISBN 978-3-540-00238-3 .
^ a b c d e f "LCDB Data for (4341) Poseidon" . Asteroid Lightcurve Database (LCDB). Retrieved 27 October 2016 .
^ a b 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 . Retrieved 27 October 2016 .
^ a b c Krugly, Yu. N.; Belskaya, I. N.; Shevchenko, V. G.; Chiorny, V. G.; Velichko, F. P.; Mottola, S.; et al. (August 2002). "The Near-Earth Objects Follow-up Program. IV. CCD Photometry in 1996-1999" . Icarus . 158 (2): 294– 304. Bibcode :2002Icar..158..294K . doi :10.1006/icar.2002.6884 . Retrieved 27 October 2016 .
^ 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 27 October 2016 .
^ a b "4341 Poseidon (1987 KF)" . Minor Planet Center . Retrieved 27 October 2016 .
^ 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 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 27 October 2016 .
External links