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2044 Wirt

From Wikipedia, the free encyclopedia
Mars-crossing asteroid binary

2044 Wirt
Discovery[1]
Discovered byC. A. Wirtanen
Discovery siteLick Obs.
Discovery date8 November 1950
Designations
(2044) Wirt
Named after
Carl Wirtanen
(discoverer himself)[2]
1950 VE
Mars-crosser[1][3] · Phocaea[4][5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.44 yr (24,269 days)
Aphelion3.1989AU
Perihelion1.5634 AU
2.3812 AU
Eccentricity0.3434
3.67yr (1,342 days)
53.286°
0° 16m 5.52s / day
Inclination23.970°
53.646°
50.474°
Knownsatellites1[6][7] (: 2 km;p: 19.0 h)
Earth MOID0.6559 AU
Physical characteristics
Dimensions6.65 km (calculated)[4]
6.66±0.6 km (IRAS:2)[8]
3.6895±0.0003h[9]
3.6898 h[10]
3.6900±0.0003 h[11]
3.690±0.00005 h[6]
0.1907±0.038 (IRAS:2)[8]
0.23 (assumed)[4]
S[4]
12.838±0.002 (R)[9] · 13.1[1][4] · 13.3[8]

2044 Wirt, provisional designation1950 VE, is abinary[7] Phocaeaasteroid andMars-crosser, approximately 6.7 kilometers in diameter. Theminor-planet moon has an estimated diameter of 1.89 kilometer.

The asteroid was discovered on 8 November 1950, by American astronomerCarl Wirtanen atLick Observatory on Mount Hamilton, California, and later named after the discoverer himself.[3]

Orbit and classification

[edit]

Wirt is both a member of the main-belt'sPhocaea family (701) and aMars-crossing asteroid, whose orbit crosses that ofMars.[1][3][4][5] It orbits the Sun in theinner main-belt at a distance of 1.6–3.2 AU once every 3 years and 8 months (1,342 days). Its orbit has aneccentricity of 0.34 and aninclination of 24° with respect to theecliptic.[1]

The asteroid'sobservation arc begins two weeks after its official discovery with the first recorded observation at Lick Observatory on 22 November 1950.[3]

Physical characteristics

[edit]

Wirt has been characterized as a stonyS-type asteroid.[4]

Rotation period

[edit]

Between 2005 and 2010, several rotationallightcurve were obtained for this asteroid from photometric observations taken by astronomersDonald Pray,Petr Pravec,Peter Kušnirák,Walter Cooney, Rui Goncalves andRaoul Behrend, as well as at thePalomar Transient Factory. The lightcurves gave a well-definedrotation period between 3.689 and 3.690 hours with a brightness variation between 0.12 and 0.26magnitude (U=n.a./3/3/3/3/2).[6][7][9][10][11]

Satellite

[edit]

During the photometric observations in December 2005, aminor-planet moon in orbit ofWirt was discovered. Thebinary asteroid has diameter ratio of 0.25, and the moon'sorbital period is 18.97 hours. It measures approximately 1.89 kilometer in diameter.[6][7][10]

Diameter and albedo

[edit]

According to the survey carried out by the Infrared Astronomical SatelliteIRAS, the asteroid measures 6.66 kilometers in diameter and its surface has analbedo of 0.19,[8] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 and calculates a diameter of 6.65 kilometers with anabsolute magnitude of 13.1.[4]

Naming

[edit]

It was named after American astronomerCarl Wirtanen (1910–1990), adiscoverer of minor planets andcomets, who was a long-time contributor ofastrometric observations at Lick Observatory. It is one of the rare cases where the asteroid had been named after its discoverer. Wirtanen is known for several surveys conducted at Lick Observatory such as theLick proper motion program with respect to galaxies and theShane-Wirtanen survey.[2] The official naming citation was published by the MPC on 1 January 1981 (M.P.C. 5688).[12]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2044 Wirt (1950 VE)" (2017-05-03 last obs.).Jet Propulsion Laboratory. Retrieved10 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(2044) Wirt".Dictionary of Minor Planet Names – (2044) Wirt.Springer Berlin Heidelberg. p. 166.doi:10.1007/978-3-540-29925-7_2045.ISBN 978-3-540-00238-3.
  3. ^abcd"2044 Wirt (1950 VE)".Minor Planet Center. Retrieved15 November 2016.
  4. ^abcdefgh"LCDB Data for (2044) Wirt". Asteroid Lightcurve Database (LCDB). Retrieved15 November 2016.
  5. ^ab"Asteroid 2044 Wirt – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  6. ^abcdPravec, P.; Scheirich, P.; Vokrouhlický, D.; Harris, A. W.; Kusnirák, P.; Hornoch, K.; et al. (March 2012)."Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries".Icarus.218 (1):125–143.Bibcode:2012Icar..218..125P.doi:10.1016/j.icarus.2011.11.026. Retrieved15 November 2016.
  7. ^abcd"Electronic Telegram No. 353". IAU Central Bureau for Astronomical Telegrams. 6 January 2006. Retrieved15 November 2016.
  8. ^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.
  9. ^abcWaszczak, 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. Retrieved15 November 2016.
  10. ^abcPray, D.; Pravec, P.; Kusnirak, P.; Cooney, W.; Gross, J.; Terrell, D.; et al. (January 2006)."(2044) Wirt".Central Bureau Electronic Telegrams.353 (353): 1.Bibcode:2006CBET..353....1P. Retrieved15 November 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2044) Wirt".Geneva Observatory. Retrieved15 November 2016.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 November 2016.


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