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F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
4827 Dares is a larger Jupiter trojan from the Trojan camp , approximately 43 kilometers (27 miles) in diameter. It was discovered on 17 August 1988 by American astronomer Carolyn Shoemaker at the Palomar Observatory in California.[1] The dark D-type asteroid has a rotation period of 19.0 hours.[7] It was named after Dares from Greek mythology.[1]
Orbit and classification
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Dares is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's L 5 Lagrangian point , 60° behind on its orbit (see Trojans in astronomy ) . It is also a non-family asteroid of the Jovian background population .[5] It orbits the Sun at a distance of 4.9–5.4 AU once every 11 years and 7 months (4,233 days; semi-major axis of 5.12 AU ). Its orbit has an eccentricity of 0.05 and an inclination of 8° with respect to the ecliptic .[3]
The body's observation arc begins with a precovery at Palomar in November 1954, almost 34 years prior to its official discovery observation.[1]
Physical characteristics
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In the SDSS -based taxonomy, Dares is a dark D-type asteroid .[10] [11] It is also characterized as a D-type by Pan-STARRS ' survey.[7] [9]
Rotation period
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In February 1994, a rotational lightcurve of Dares was obtained over five nights of observation by Stefano Mottola and Anders Erikson using the ESO 1-metre telescope at La Silla Observatory in Chile. Lightcurve analysis showed a well-defined rotation period of 18.995± 0.028 hours with a brightness variation of 0.24 magnitude (U=3 ).[7] [8]
In October 2013, photometric observations in the R-band by astronomers at the Palomar Transient Factory in California gave a concurring period of 18.967 hours with an amplitude of 0.23 magnitude (U=2 ).[7] [12]
Diameter and albedo
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According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Dares measures 42.77 kilometers in diameter and its surface has an albedo of 0.067,[6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 44.22 kilometers based on an absolute magnitude of 10.5.[7]
Naming
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This minor planet was named by the discoverer from Greek mythology after the Trojan Dares , one of Aeneas ' wandering companions (Aeneads ) who were not killed or enslaved by the end of the Trojan War .[1] The official naming citation was published by the Minor Planet Center on 25 August 1991 (M.P.C. 18647 ).[13]
References
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^ Noah Webster (1884) A Practical Dictionary of the English Language
^ a b c d "JPL Small-Body Database Browser: 4827 Dares (1988 QE)" (2018-05-22 last obs.). Jet Propulsion Laboratory . Retrieved 21 June 2018 .
^ "List of Jupiter Trojans" . Minor Planet Center . 1 June 2018. Retrieved 21 June 2018 .
^ a b "Asteroid (4827) Dares – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 21 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 . (online catalog )
^ a b c d e f g h i "LCDB Data for (4827) Dares" . Asteroid Lightcurve Database (LCDB). Retrieved 21 June 2018 .
^ 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 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 "Asteroid 4827 Dares" . Small Bodies Data Ferret . Retrieved 21 June 2018 .
^ 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 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 21 June 2018 .
External links
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R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=4827_Dares&oldid=1191443427 "
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