astro.wikisort.org - Asteroid
Hermione (minor planet designation: 121 Hermione) is a very large binary asteroid discovered in 1872. It orbits in the Cybele group in the far outer asteroid belt.[13] As an asteroid of the dark C spectral type, it is probably composed of carbonaceous materials. In 2002, a small moon was found to be orbiting Hermione.[13]
 121 Hermione and its moon | |
| Discovery[1] | |
|---|---|
| Discovered by | James Craig Watson |
| Discovery date | 12 May 1872 |
| Designations | |
MPC designation | (121) Hermione |
| Pronunciation | /hɜːrˈmaɪ.əniː/[2] |
Named after | Hermione[3] (Greek mythology) |
Alternative designations | A872 JA; 1970 VE |
Minor planet category | main-belt · Cybele |
| Adjectives | Hermionean /hɜːrmaɪ.əˈniːən/ |
| Orbital characteristics[4] | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 145.96 yr (53,312 d) |
| Aphelion | 3.9067 AU |
| Perihelion | 2.9889 AU |
Semi-major axis | 3.4478 AU |
| Eccentricity | 0.1331 |
Orbital period (sidereal) | 6.40 yr (2,338 d) |
Mean anomaly | 157.08° |
Mean motion | 0° 9m 14.4s / day |
| Inclination | 7.5975° |
Longitude of ascending node | 73.127° |
Argument of perihelion | 298.18° |
| Known satellites | S/2002 (121) 1 |
| Physical characteristics | |
| Dimensions | 268×186×183 km[5] 254±4 × 125±9 km[6] |
Mean radius | 95 km[6] |
| Mass | 5.38 ± 0.3 ×1018 kg[5] 5.4 ± 0.3×1018 kg[7] |
Mean density | 1.13 ± 0.3 g/cm3[5] 1.8 ± 0.2 g/cm3[7][8] |
Equatorial surface gravity | 0.022 m/s2[9] |
Equatorial escape velocity | 0.075 km/s[9] |
Sidereal rotation period | 0.2313 d (5.551 h)[10] |
Axial tilt | 73° |
Pole ecliptic latitude | +10 ± 2°[7] |
Pole ecliptic longitude | 1.5 ± 2° |
Geometric albedo | 0.0482 ± 0.002[11] |
Spectral type | C[12] |
Absolute magnitude (H) | 7.31[11] |
Discovery
Hermione was discovered by J. C. Watson on 12 May 1872 from Ann Arbor, Michigan, in the United States,[13] and named after Hermione, daughter of Menelaus and Helen in Greek mythology.[3]
Physical properties
The asteroid has a bi-lobed shape, as evidenced by adaptive optics images, the first of which were taken in December 2003 with the Keck telescope.[6] Of several proposed shape models that agreed with the images, a "snowman"-like shape was found to best fit the observed precession rate of Hermione's satellite.[7] In this "snowman" model, the asteroid's shape can be approximated by two partially overlapping spheres of radii 80 and 60 km, whose centers are separated by a distance of 115 km. A simple ellipsoid shape was ruled out.
Observation of the satellite's orbit has made possible an accurate determination of Hermione's mass.[7] For the best-fit "snowman" model, the density is found to be 1.8 ± 0.2 g/cm3, giving a porosity on the order of 20%, and possibly indicating that the main components are fractured solid bodies, rather than the asteroid being a rubble pile.
Occultations by Hermione have been successfully observed three times so far, the last time in February 2004.
| Discovery[14] | |
|---|---|
| Discovered by | W. J. Merline, P. M. Tamblyn, C. Dumas, L. M. Close, C. R. Chapman, F. Menard, W. M. Owen, and D. C. Slater |
| Discovery date | 2002-09-28 |
| Designations | |
Alternative designations | LaFayette |
Minor planet category | main-belt · Cybele |
| Orbital characteristics[15] | |
Semi-major axis | 768 ± 11 km |
| Eccentricity | 0.001 ± 0.001 |
Orbital period (sidereal) | 2.582 ± 0.002 d |
| Inclination | 3 ± 2° (with respect to Hermione pole) |
| Satellite of | 121 Hermione |
| Physical characteristics | |
| Dimensions | 12 ± 4 km[6] |
| Mass | ~1.6×1015 kg[16] |
Absolute magnitude (H) | 13.0[6] |
Moon
A satellite of Hermione was discovered in 2002 with the Keck II telescope.[13] It is about 8 miles (13 km) in diameter.[13] The satellite is provisionally designated S/2002 (121) 1. It has not yet been officially named, but "LaFayette" has been proposed by a group of astronomers in reference to the frigate used in secret by the Marquis de Lafayette to reach America to help the insurgents.[17][6]
References
- "121 Hermione". Minor Planet Center. Retrieved 14 September 2018.
- Noah Webster (1884) A Practical Dictionary of the English Language
- Schmadel, Lutz D. (2007). "(121) Hermione". Dictionary of Minor Planet Names – (121) Hermione. Springer Berlin Heidelberg. p. 26. doi:10.1007/978-3-540-29925-7_122. ISBN 978-3-540-00238-3.
- "JPL Small-Body Database Browser: 121 Hermione" (2018-05-25 last obs.). Jet Propulsion Laboratory. Retrieved 14 September 2018.
- Jim Baer (2008). "Recent Asteroid Mass Determinations". Personal Website. Archived from the original on 2 July 2013. Retrieved 7 December 2008.
- F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.
- F. Marchis; et al. (2005). "Mass and density of Asteroid 121 Hermione from an analysis of its companion orbit". Icarus. 178 (2): 450–464. Bibcode:2005Icar..178..450M. doi:10.1016/j.icarus.2005.05.003.
- Using the "snowman" shape model, which best matches the value of J2 implied from precession.
- On the extremities of the long axis.
- IAUC 8264 Archived 9 July 2008 at the Wayback Machine
- Supplemental IRAS minor planet survey Archived 2009-08-17 at the Wayback Machine
- PDS node taxonomy database Archived 2009-08-05 at the Wayback Machine
- Linda T. Elkins-Tanton (2010). Asteroids, Meteorites, and Comets. Infobase Publishing. p. 96. ISBN 978-1-4381-3186-3.
- IAUC 7980 Archived 2006-05-01 at the Wayback Machine
- 121 Hermione and S/2002 (121) 1, orbit data website maintained by F. Marchis.
- Assuming a similar density to the primary.
- Johnston, Wm. Robert (21 September 2014). "(121) Hermione and S/2002 (121) 1 ("LaFayette")". Asteroids with Satellites Database. Johnston's Archive. Retrieved 7 November 2021.
External links
- 121 Hermione and S/2002 (121) 1, orbit data website maintained by F. Marchis. Includes adaptive optics images, orbit diagrams, and shape models.
- (121) Hermione, datasheet, johnstonsarchive.net
- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- Tally of Asteroids Harboring Moons Grows Beyond 30 (Space.com, 3 October 2002)
- 121 Hermione at AstDyS-2, Asteroids—Dynamic Site
- 121 Hermione at the JPL Small-Body Database
На других языках
[de] (121) Hermione
(121) Hermione ist ein Asteroid des äußeren Asteroiden-Hauptgürtels. Mit einem mittleren Durchmesser von 187 km gehört er zu den größten Asteroiden des Hauptgürtels und hat einen vergleichsweise großen Mond mit der Bezeichnung S/2002 (121) 1.- [en] 121 Hermione
[es] (121) Hermione
(121) Hermione es un asteroide perteneciente al cinturón exterior de asteroides descubierto por James Craig Watson el 12 de mayo de 1872 desde el observatorio Detroit de Ann Arbor, Estados Unidos. Está nombrado por Hermíone, un personaje de la mitología griega.[2][ru] (121) Гермиона
(121) Гермиона (др.-греч. Ἑρμιόνη) — очень крупный астероид внешней части главного пояса, который принадлежит к тёмному спектральному классу C и входит в состав семейства Кибелы. Он был обнаружен 12 мая 1872 года американским астрономом Дж. К. Уотсоном в Энн-Арбор, США и назван в честь Гермионы, дочери царя Спарты Менелая и Елены[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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