astro.wikisort.org - Asteroid
10502 Armaghobs (/ɑːrˈmɑːəbz/ ar-MAH-əbz), provisional designation 1987 QF6, is an eccentric, rare-type stony asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 2.6 kilometers in diameter. The asteroid was discovered on 22 August 1987, by American astronomer Eleanor Helin at the Palomar Observatory in California, United States.[7] It was named for the Armagh Observatory in Northern Ireland.[2]
| Discovery[1] | |
|---|---|
| Discovered by | E. F. Helin |
| Discovery site | Palomar Obs. |
| Discovery date | 22 August 1987 |
| Designations | |
MPC designation | (10502) Armaghobs |
| Pronunciation | /ɑːrˈmɑːəbz/ ar-MAH-əbs |
Named after | Armagh Observatory (in Northern Ireland)[2] |
Alternative designations | 1987 QF6 · 1980 PJ2 1994 RJ29 |
Minor planet category | Mars-crosser[3] |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 36.73 yr (13,416 days) |
| Aphelion | 3.0439 AU |
| Perihelion | 1.5745 AU |
Semi-major axis | 2.3092 AU |
| Eccentricity | 0.3182 |
Orbital period (sidereal) | 3.51 yr (1,282 days) |
Mean anomaly | 145.86° |
Mean motion | 0° 16m 51.24s / day |
| Inclination | 21.927° |
Longitude of ascending node | 170.23° |
Argument of perihelion | 263.26° |
| Physical characteristics | |
| Dimensions | 2.61±0.59 km[4] 2.97 km (calculated)[3] |
Synodic rotation period | 24.978±0.002 h[5] |
Geometric albedo | 0.20 (assumed)[3] 0.22±0.14[4] |
Spectral type | S[3] · Q[6] |
Absolute magnitude (H) | 15.0[1][3] · 15.18 · 15.44±0.08[6] |
Orbit and classification
Armaghobs orbits the Sun in the inner main-belt at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,282 days). Its orbit has an eccentricity of 0.32 and an inclination of 22° with respect to the ecliptic.[1] It was first identified as 1980 PJ2 at ESO's La Silla Observatory in 1980, extending the body's observation arc by 7 years prior to its official discovery observation at Palomar.[7]
Physical characteristics
The Armaghobs has been characterized as a relatively rare Q-type asteroid by Pan-STARRS photometric survey.[6]
Lightcurve
In February 2013, a rotational lightcurve of Armaghobs was obtained from photometric observations by Kevin Hills at the Riverland Dingo Observatory at Moorook, South Australia. Lightcurve analysis gave a rotation period of 24.978 hours with a brightness variation of 0.51 magnitude (U=2).[5]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Armaghobs measures 2.61 kilometers in diameter and its surface has an albedo of 0.22.[4] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20, and calculates a diameter of 2.97 kilometers with an absolute magnitude of 15.0.[3]
Naming
This minor planet was named after the Armagh Observatory in Northern Ireland. The present-day astronomical research institute was founded by Archbishop Richard Robinson in 1790. The Estonian astronomer Ernst Öpik, after whom 2099 Öpik is named, had been a long-time member of the Observatory. It is also known for the invention of the cup-anemometer by Thomas Robinson, the New General Catalogue compiled by John Dreyer, and Lindsay's Armagh-Dunsink-Harvard telescope.[2] The official naming citation was published by the Minor Planet Center on 9 January 2001 (M.P.C. 41937).[8]
References
- "JPL Small-Body Database Browser: 10502 Armaghobs (1987 QF6)" (2017-05-04 last obs.). Jet Propulsion Laboratory. Retrieved 23 June 2017.
- Schmadel, Lutz D. (2007). "(10502) Armaghobs". Dictionary of Minor Planet Names – (10502) Armaghobs. Springer Berlin Heidelberg. p. 736. doi:10.1007/978-3-540-29925-7_8003. ISBN 978-3-540-00238-3.
- "LCDB Data for (10502) Armaghobs". Asteroid Lightcurve Database (LCDB). Retrieved 28 April 2016.
- 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 23 June 2017.
- Hills, Kevin (January 2014). "Asteroid Lightcurve Analysis at Riverland Dingo Observatory (RDO): 2013 Results". The Minor Planet Bulletin. 41 (1): 2–3. Bibcode:2014MPBu...41....2H. ISSN 1052-8091. Retrieved 28 April 2016.
- 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. Retrieved 28 April 2016.
- "10502 Armaghobs (1987 QF6)". Minor Planet Center. Retrieved 28 April 2016.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 28 April 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
- 10502 Armaghobs at AstDyS-2, Asteroids—Dynamic Site
- 10502 Armaghobs at the JPL Small-Body Database
На других языках
- [en] 10502 Armaghobs
[ru] (10502) Арманобс
(10502) Арманобс (лат. Armaghobs) — астероид, относящийся к группе астероидов, пересекающих орбиту Марса, который принадлежит к редкому спектральному классу Q[3]. Он был открыт 22 августа 1987 года американским астрономом Элеанор Хелин в Паломарской обсерватории и назван в честь Арманской обсерватории в Северной Ирландии[4]. Название было утверждено и опубликовано 9 января 2001 года[5].Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
WikiSort.org - проект по пересортировке и дополнению контента Википедии