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1345 Potomac

From Wikipedia, the free encyclopedia
Hildian asteroid

1345 Potomac
Discovery[1]
Discovered byJ. H. Metcalf
Discovery siteTaunton Obs.
Discovery date4 February 1908
Designations
(1345) Potomac
Named after
Potomac River[2]
(U.S. Mid-Atlanticriver)
1908 CG · 1932 CF
1932 EA · 1932 FB
1971 DE2
main-belt · (outer)[3]
Hilda[1][4] · background[5]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc111.20yr (40,617 d)
Aphelion4.7100AU
Perihelion3.2611 AU
3.9856 AU
Eccentricity0.1818
7.96 yr (2,906 d)
31.380°
0° 7m 26.04s / day
Inclination11.402°
137.43°
333.12°
Jupiter MOID0.4592 AU
TJupiter2.9930
Physical characteristics
71.82±3.0 km[6]
72.975±0.463 km[7]
76.72±2.34 km[8]
11.41±0.01 h[9]
0.039±0.003[8]
0.043±0.008[7]
0.0439±0.004[6]
Tholen =X[3] · C[4][10]
B–V = 0.719[3]
U–B = 0.286[3]
9.73[3][4][6][8]
9.9[1]

1345 Potomac (/pəˈtmək/ ), provisional designation1908 CG, is a darkHildianasteroid from the outermost regions of theasteroid belt, approximately 73 kilometers (45 mi) in diameter. It was discovered on 4 February 1908, by American astronomerJoel Metcalf at the Taunton Observatory (803) in Massachusetts, United States.[1] TheX-type asteroid has arotation period of 11.4 hours.[4] It was named for thePotomac River on which Washington, D.C. is located.[2]

Orbit and classification

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Potomac is member of the dynamicalHilda group, which stays in 3:2orbital resonance with Jupiter.[1][4] It is, however, not a member of theHilda family but a non-family asteroid of the main belt'sbackground population when applying theHierarchical Clustering Method to itsproper orbital elements.[5]

It orbits the Sun in theoutermost 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 aneccentricity of 0.18 and aninclination of 11° with respect to theecliptic.[3] The body'sobservation arc begins at theUnited States Naval Observatory, three weeks after its official discovery observation at Taunton.[1]

Naming

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Thisminor 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 theChesapeake Bay and forms the southern boundary ofMaryland. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 122).[2]

Physical characteristics

[edit]

In theTholen classification,Potomac is anX-type asteroid.[3] It has also been characterized as a carbonaceousC-type asteroid byPan-STARRS photometric survey.[10]

Rotation period

[edit]

Two rotationallightcurves ofPotomac was obtained from photometric observations. Lightcurve analysis gave arotation period of 11.40 and 11.41 hours with a brightness amplitude of 0.22 and 0.24magnitude, respectively (U=2/3).[11][9]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Potomac measures between 71.82 and 76.72 kilometers in diameter and its surface has analbedo between 0.039 and 0.0439.[6][7][8]

TheCollaborative 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 anabsolute magnitude of 9.73.[4]

References

[edit]
  1. ^abcdef"1345 Potomac (A908 CE)".Minor Planet Center. Retrieved29 October 2019.
  2. ^abcSchmadel, 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.
  3. ^abcdefgh"JPL Small-Body Database Browser: 1345 Potomac (A908 CE)" (2019-05-10 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 August 2020. Retrieved29 October 2019.
  4. ^abcdef"LCDB Data for (1345) Potomac". Asteroid Lightcurve Database (LCDB). Retrieved17 November 2017.
  5. ^ab"Asteroid 1345 Potomac – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcdTedesco, 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. Retrieved22 October 2019.
  7. ^abcGrav, 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. Retrieved17 November 2017.
  8. ^abcdUsui, 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)
  9. ^abBrinsfield, 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. Retrieved17 November 2017.
  10. ^abVeres, 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. Retrieved17 November 2017.
  11. ^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. Retrieved17 November 2017.

External links

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