astro.wikisort.org - Asteroid
Olga (minor planet designation: 304 Olga) is a large Main belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
| Discovery | |
|---|---|
| Discovered by | Johann Palisa |
| Discovery date | 14 February 1891 |
| Designations | |
MPC designation | (304) Olga |
| Pronunciation | /ˈɒlɡə/, German: [ˈɔlɡaː][1] |
Minor planet category | Main belt |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 124.78 yr (45577 d) |
| Aphelion | 2.93719 AU (439.397 Gm) |
| Perihelion | 1.86853 AU (279.528 Gm) |
Semi-major axis | 2.40286 AU (359.463 Gm) |
| Eccentricity | 0.22237 |
Orbital period (sidereal) | 3.72 yr (1360.5 d) |
Mean anomaly | 63.6148° |
Mean motion | 0° 15m 52.607s / day |
| Inclination | 15.8530° |
Longitude of ascending node | 159.080° |
Argument of perihelion | 172.423° |
| Physical characteristics | |
| Dimensions | 67.86±2.1 km[2] 70.30 ± 2.32 km[3] |
| Mass | (1.15 ± 1.12) × 1018 kg[3] |
Synodic rotation period | 18.36 h (0.765 d) |
Geometric albedo | 0.0488±0.003 |
Spectral type | C |
Absolute magnitude (H) | 9.74 |
It was discovered by Johann Palisa on 14 February 1891 in Vienna.
304 Olga was identified as one of three asteroids that were likely to be a parent body for chondrites along with 449 Hamburga and 335 Roberta.[4] All three asteroids were known to have low-albedo (not reflect as much light) and be close to "meteorite producing resonances".[4] Chrondrites are the most common type of meteor found on Earth, accounting for over 80% of all meteors.[5] They are named for the tiny spherical silicate particles that are found inside them (those particles are called chondrules).[5]
- Orbit diagram
References
- (German Names)
- "304 Olga". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- Lunar and planetary science: abstracts of papers submitted to the ... Lunar and Planetary Science Conference. Lunar and Planetary Institute. 1996.
- "ASU - Chondrites". Archived from the original on 22 June 2019. Retrieved 31 August 2015.
External links
- 304 Olga at AstDyS-2, Asteroids—Dynamic Site
- 304 Olga at the JPL Small-Body Database
 | This article about a C-type asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |
На других языках
[de] (304) Olga
(304) Olga ist ein Asteroid des Asteroiden-Hauptgürtels, der am 14. Februar 1891 von Johann Palisa am Observatorium von Wien entdeckt wurde.- [en] 304 Olga
[es] (304) Olga
(304) Olga es un asteroide perteneciente al cinturón de asteroides descubierto el 14 de febrero de 1891 por Johann Palisa desde el observatorio de Viena, Austria. Está nombrado en honor de una sobrina del astrónomo alemán Friedrich Argelander.[2][ru] (304) Ольга
(304) Ольга (нем. Olga) — астероид главного пояса, который принадлежит к тёмному спектральному классу C и состоит простейших углеродных соединений. Он был открыт 14 февраля 1891 года австрийским астрономом Иоганном Пализой в обсерватории Вены и назван в честь племянницы прусского астронома Фридриха Аргеландера[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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