astro.wikisort.org - Asteroid2937 Gibbs, provisional designation 1980 LA, is a stony Phocaea asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 14 June 1980, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station near Flagstaff, Arizona.[3] The asteroid was named after American scientist Josiah Willard Gibbs.[2]
Asteroid
2937 Gibbs|
Discovered by | E. Bowell |
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Discovery site | Anderson Mesa Stn. |
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Discovery date | 14 June 1980 |
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MPC designation | (2937) Gibbs |
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Named after | Josiah Willard Gibbs [2] (American scientist) |
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Alternative designations | 1980 LA |
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Minor planet category | Mars-crosser [1][3] · Phocaea [4][5] |
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Epoch 4 September 2017 (JD 2458000.5) |
Uncertainty parameter 0 |
Observation arc | 36.75 yr (13,424 days) |
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Aphelion | 3.0232 AU |
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Perihelion | 1.6160 AU |
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Semi-major axis | 2.3196 AU |
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Eccentricity | 0.3033 |
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Orbital period (sidereal) | 3.53 yr (1,290 days) |
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Mean anomaly | 161.70° |
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Mean motion | 0° 16m 44.4s / day |
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Inclination | 21.758° |
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Longitude of ascending node | 265.72° |
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Argument of perihelion | 71.849° |
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Dimensions | 5.04±1.43 km[6] 5.99±1.20 km[7] 6.35 km (calculated)[4] |
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Synodic rotation period | 3.06±0.05 h[8] 3.06153±0.00006 h[8] 3.189±0.003 h[9][lower-alpha 1] |
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Geometric albedo | 0.23 (assumed)[4] 0.283±0.113[7] 0.30±0.13[6] |
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Spectral type | S [4] |
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Absolute magnitude (H) | 13.10[7] · 13.2[1][4] · 13.42[6] |
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Orbit and classification
Gibbs is a Mars-crossing asteroid, as it crosses the orbit of Mars at 1.666 AU.[1][3] It is also an eccentric member of the Phocaea family,[4][5] a large asteroid family of stony asteroids in the inner main-belt.[10]: 23 Gibbs orbits the Sun at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,290 days). Its orbit has an eccentricity of 0.30 and an inclination of 22° with respect to the ecliptic.[1]
The asteroid's observation arc begins with its official discovery observation at Anderson Mesa. No prior identifications were made and no precoveries taken.[3]
Physical characteristics
Gibbs is an assumed stony S-type asteroid, which agrees with the overall spectral type of the Phocaea family.[10]: 23
Rotation period
In 2005, two rotational lightcurves of Gibbs were obtained from photometric observations by Italian amateur astronomers Federico Manzini and Roberto Crippa. Lightcurve analysis gave a rotation period of 3.06 and 3.06153 hours with a brightness variation of 0.31 and 0.39 magnitude, respectively (U=2/3-).[8] In December 2016, Robert Stephens obtained a well-defined lightcurve at his Trojan Station (U81) that gave a period of 3.189 hours and an amplitude of 0.26 magnitude (U=3).[9][lower-alpha 1]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Gibbs measures between 5.04 and 5.99 kilometers in diameter and its surface has an albedo between 0.283 and 0.30,[6][7] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from 25 Phocaea, the Phocaea family's largest member and namesake – and calculates a diameter of 6.35 kilometers based on an absolute magnitude of 13.2.[4]
Naming
This minor planet was named in memory of American mathematician and physicist Josiah Willard Gibbs (1839–1903), who contributed to the studies of asteroids through his work on orbits.[2] The official naming citation was published by the Minor Planet Center on 17 February 1984 (M.P.C. 8544).[11] The lunar crater Gibbs was also named in his honor.[2]
Notes
- Lightcurve plot for (2937) Gibbs. Robert D. Stephens (2016). Rotation period of 3.189±0.003 hours with a brightness amplitude of 0.26 mag. Quality Code of 3. Summary figures at the CS3 website and at the LCDB
References
- "JPL Small-Body Database Browser: 2937 Gibbs (1980 LA)" (2017-03-16 last obs.). Jet Propulsion Laboratory. Retrieved 15 September 2017.
- Schmadel, Lutz D. (2007). "(2937) Gibbs". Dictionary of Minor Planet Names – (2937) Gibbs. Springer Berlin Heidelberg. pp. 241–242. doi:10.1007/978-3-540-29925-7_2938. ISBN 978-3-540-00238-3.
- "2937 Gibbs (1980 LA)". Minor Planet Center. Retrieved 15 September 2017.
- "LCDB Data for (2937) Gibbs". Asteroid Lightcurve Database (LCDB). Retrieved 15 September 2017.
- "Asteroid 2937 Gibbs – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
- Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63. Retrieved 15 September 2017.
- Alí-Lagoa, V.; Delbo', M. (July 2017). "Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data". Astronomy and Astrophysics. 603: 8. arXiv:1705.10263. Bibcode:2017A&A...603A..55A. doi:10.1051/0004-6361/201629917.
- Behrend, Raoul. "Asteroids and comets rotation curves – (2937) Gibbs". Geneva Observatory. Retrieved 15 September 2017.
- Stephens, Robert D. (April 2017). "Asteroids Observed from CS3: 2016 October - December". The Minor Planet Bulletin. 44 (2): 120–122. Bibcode:2017MPBu...44..120S. ISSN 1052-8091. Retrieved 15 September 2017.
- Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). Identification and Dynamical Properties of Asteroid Families. Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 15 September 2017.
External links
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- 2936 Nechvíle
- 2937 Gibbs
- 2938 Hopi
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На других языках
[de] (2937) Gibbs
(2937) Gibbs (1980 LA) ist ein ungefähr fünf Kilometer großer Asteroid des inneren Hauptgürtels, der am 14. Juni 1980 vom US-amerikanischen Astronomen Edward L. G. Bowell am Lowell-Observatorium, Anderson Mesa Station (Anderson Mesa) in der Nähe von Flagstaff, Arizona (IAU-Code 688) entdeckt wurde.
- [en] 2937 Gibbs
[ru] (2937) Гиббс
(2937) Гиббс (лат. Gibbs) — небольшой астероид, который относится к группе астероидов пересекающих орбиту Марса. Он был открыт 14 июня 1980 года американским астрономом Эдвардом Боуэллом в обсерватории Андерсон Меса и назван в честь известного американского учёного Джозайя Гиббса[1].
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