astro.wikisort.org - Asteroid
2099 Öpik, provisional designation 1977 VB, is a dark and eccentric asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 5.1 kilometers in diameter.
| Discovery [1] | |
|---|---|
| Discovered by | E. F. Helin |
| Discovery site | Palomar Obs. |
| Discovery date | 8 November 1977 |
| Designations | |
MPC designation | (2099) Opik |
Named after | Ernst Öpik (Estonian astronomer)[2] |
Alternative designations | 1977 VB · 1977 UL2 |
Minor planet category | Mars-crosser [1][3] |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 60.26 yr (22,009 days) |
| Aphelion | 3.1370 AU |
| Perihelion | 1.4710 AU |
Semi-major axis | 2.3040 AU |
| Eccentricity | 0.3616 |
Orbital period (sidereal) | 3.50 yr (1,277 days) |
Mean anomaly | 148.76° |
Mean motion | 0° 16m 54.48s / day |
| Inclination | 26.966° |
Longitude of ascending node | 218.84° |
Argument of perihelion | 159.18° |
| Earth MOID | 0.4926 AU |
| Physical characteristics | |
| Dimensions | 5.12 km (calculated)[4] 5.17±1.35 km[5] |
Synodic rotation period | 6.4430±0.0002 h[6] 9.3 h[7] |
Geometric albedo | 0.05±0.06[5] 0.057 (assumed)[4] |
Spectral type | S (Tholen)[1] Ch (SMASS)[1] C (CALL)[4] B–V = 0.690[1] U–B = 0.350[1] |
Absolute magnitude (H) | 15.18[1][4] · 15.22[5] |
The asteroid was discovered on 8 November 1977, by American astronomer Eleanor Helin at the Palomar Observatory in California, and named after Estonian astronomer Ernst Öpik.[3]
Orbit and classification
Öpik orbits the Sun in the inner main-belt at a distance of 1.5–3.1 AU once every 3 years and 6 months (1,277 days). Its orbit has an eccentricity of 0.36 and an inclination of 27° with respect to the ecliptic.[1] The first used precovery was taken at the discovering observatory in 1970, extending the asteroid's observation arc by 7 years prior to its discovery.[3]
Physical characteristics
Originally, the asteroid's spectral type was that of a bright S-type asteroid in the Tholen classification. More recently, it has been characterized as a dark Ch-type, a hydrated subtype of the carbonaceous C-type asteroids in the SMASS classification, which is in agreement with its low albedo (below).[1]
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Öpik measures 5.17 kilometers in diameter and its surface has an albedo of 0.05.[5] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 5.12 kilometers with an absolute magnitude of 15.18.[4]
Rotation period
In 2005, a photometric lightcurve analysis by several astronomers including Pierre Antonini, rendered a rotation period of 6.4430±0.0002 hours and with a brightness amplitude of 0.21 in magnitude (U=2),[6] superseding the results of an observation from the 1990s that gave a longer period of 9.3 hours (U=2).[7]
Naming
This minor planet was named after Estonian astronomer and astrophysicist, Ernst Öpik (1893–1985), who has influenced many fields of astronomy during his 60-year long career. He is noted for developing the discipline of statistical celestial mechanics and for methods to estimate the lifetimes of planet-crossing asteroids. In the early 1950s, he calculated the impact probability of Mars-crossing asteroids with Mars, and concluded that a search for impact craters on Mars would be a fruitful. Fourteen years later, Martian craters were discovered by Mariner 4.[2] The official naming citation was published by the Minor Planet Center on 1 November 1978 (M.P.C. 4548).[8]
References
- "JPL Small-Body Database Browser: 2099 Opik (1977 VB)" (2017-03-05 last obs.). Jet Propulsion Laboratory. Retrieved 11 June 2017.
- Schmadel, Lutz D. (2007). "(2099) Öpik". Dictionary of Minor Planet Names – (2099) Öpik. Springer Berlin Heidelberg. p. 170. doi:10.1007/978-3-540-29925-7_2100. ISBN 978-3-540-00238-3.
- "2099 Opik (1977 VB)". Minor Planet Center. Retrieved 7 December 2016.
- "LCDB Data for (2099) Öpik". Asteroid Lightcurve Database (LCDB). Retrieved 7 December 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 11 June 2017.
- Behrend, Raoul. "Asteroids and comets rotation curves – (2099) Öpik". Geneva Observatory. Retrieved 7 December 2016.
- Goretti, V. (December 2000). "CCD Photometry of the Mars-crosser Asteroid 2099 Opik". The Minor Planet Bulletin. 27: 46. Bibcode:2000MPBu...27...46G. Retrieved 27 April 2016.
- Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN 978-3-642-01964-7.
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 (1)-(5000) – Minor Planet Center
- 2099 Öpik at AstDyS-2, Asteroids—Dynamic Site
- 2099 Öpik at the JPL Small-Body Database
На других языках
[de] (2099) Öpik
(2099) Öpik (1977 VB; 1977 UL2) ist ein Asteroid des inneren Hauptgürtels, der am 8. November 1977 von Eleanor Helin am Palomar-Observatorium entdeckt wurde.- [en] 2099 Öpik
[ru] (2099) Эпик
(2099) Эпик (эст. Öpik) — астероид, относящийся к группе астероидов пересекающих орбиту Марса, который принадлежит к тёмному спектральному классу C. Он был открыт 8 ноября 1977 года американским астрономом Элеанорой Хелин в Паломарской обсерватории и назван в честь эстонского астронома Эрнста Эпика[1].Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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