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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
1345 Potomac (), provisional designation 1908 CG , is a dark Hildian asteroid from the outermost regions of the asteroid belt , approximately 73 kilometers (45 mi ) in diameter. It was discovered on 4 February 1908, by American astronomer Joel Metcalf at the Taunton Observatory (803 ) in Massachusetts, United States.[1] The X-type asteroid has a rotation period of 11.4 hours.[4] It was named for the Potomac River on which Washington, D.C. is located.[2]
Orbit and classification [ edit ]
Potomac is member of the dynamical Hilda group , which stays in 3:2 orbital resonance with Jupiter.[1] [4] It is, however, not a member of the Hilda family but a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements .[5]
It orbits the Sun in the outermost asteroid belt at a distance of 3.3–4.7 AU once every 7 years and 12 months (2,910 days; semi-major axis of 3.99 AU ). Its orbit has an eccentricity of 0.18 and an inclination of 11° with respect to the ecliptic .[3] The body's observation arc begins at the United States Naval Observatory , three weeks after its official discovery observation at Taunton.[1]
This minor planet was named after the U.S. Potomac River in the Mid-Atlantic region of the United States, on which Washington, D.C. is located. The river flows from West Virginia into the Chesapeake Bay and forms the southern boundary of Maryland . The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 122 ).[2]
Physical characteristics [ edit ]
In the Tholen classification , Potomac is an X-type asteroid .[3] It has also been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey.[10]
Rotation period [ edit ]
Two rotational lightcurves of Potomac was obtained from photometric observations. Lightcurve analysis gave a rotation period of 11.40 and 11.41 hours with a brightness amplitude of 0.22 and 0.24 magnitude , respectively (U=2/3 ).[11] [9]
Diameter and albedo [ edit ]
According to the surveys carried out by the Infrared Astronomical Satellite IRAS , the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Potomac measures between 71.82 and 76.72 kilometers in diameter and its surface has an albedo between 0.039 and 0.0439.[6] [7] [8]
The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0439 and a diameter of 71.82 kilometers based on an absolute magnitude of 9.73.[4]
References [ edit ]
^ a b c Schmadel, Lutz D. (2007). "(1345) Potomac". Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 109. doi :10.1007/978-3-540-29925-7_1346 . ISBN 978-3-540-00238-3 .
^ a b c d e f g h "JPL Small-Body Database Browser: 1345 Potomac (A908 CE)" (2019-05-10 last obs.). Jet Propulsion Laboratory . Archived from the original on 20 August 2020. Retrieved 29 October 2019 .
^ a b c d e f "LCDB Data for (1345) Potomac" . Asteroid Lightcurve Database (LCDB). Retrieved 17 November 2017 .
^ a b "Asteroid 1345 Potomac – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019 .
^ 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 . 12 : IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode :2004PDSS...12.....T . Retrieved 22 October 2019 .
^ a b c Grav, T.; Mainzer, A. K.; Bauer, J.; Masiero, J.; Spahr, T.; McMillan, R. S.; et al. (January 2012). "WISE/NEOWISE Observations of the Hilda Population: Preliminary Results" . The Astrophysical Journal . 744 (2 ): 15. arXiv :1110.0283 . Bibcode :2012ApJ...744..197G . doi :10.1088/0004-637X/744/2/197 . S2CID 44000310 . Retrieved 17 November 2017 .
^ 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 )
^ a b Brinsfield, James W. (April 2010). "Asteroid Lightcurve Analysis at Via Capote Observatory: 4th Quarter 2009" . The Minor Planet Bulletin . 37 (2 ): 50–53. Bibcode :2010MPBu...37...50B . ISSN 1052-8091 . Retrieved 17 November 2017 .
^ 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 . Retrieved 17 November 2017 .
^ Dahlgren, M.; Lahulla, J. F.; Lagerkvist, C.-I.; Lagerros, J.; Mottola, S.; Erikson, A.; et al. (June 1998). "A Study of Hilda Asteroids. V. Lightcurves of 47 Hilda Asteroids" . Icarus . 133 (2 ): 247–285. Bibcode :1998Icar..133..247D . doi :10.1006/icar.1998.5919 . Retrieved 17 November 2017 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=1345_Potomac&oldid=1209750030 "
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