astro.wikisort.org - Asteroid711 Marmulla is an asteroid belonging to the Flora family in the Main Belt.[2] It was discovered 1 March 1911 by Austrian astronomer Johann Palisa. The asteroid name may be derived from the Old High German word 'marmul', which means 'marble'.[3] This asteroid is orbiting 2.24 AU from the Sun with a period of 3.35 yr and an eccentricity (ovalness) of 0.195. The orbital plane of 711 Marmulla is inclined at an angle of 6.1° to the plane of the ecliptic.[1]
711 Marmulla|
Discovered by | J. Palisa |
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Discovery site | Vienna Obs. |
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Discovery date | 1 March 1911 |
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MPC designation | (711) Marmulla |
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Pronunciation | |
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Alternative designations | 1911 LN; 1927 AB |
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Epoch 31 July 2016 (JD 2457600.5) |
Uncertainty parameter 0 |
Observation arc | 102.99 yr (37,618 d) |
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Aphelion | 2.6745 AU (400.10 Gm) |
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Perihelion | 1.8003 AU (269.32 Gm) |
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Semi-major axis | 2.2374 AU (334.71 Gm) |
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Eccentricity | 0.19535 |
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Orbital period (sidereal) | 3.35 yr (1,222.4 d) |
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Mean anomaly | 65.0629° |
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Mean motion | 0° 17m 40.2s / day |
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Inclination | 6.0917° |
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Longitude of ascending node | 357.091° |
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Argument of perihelion | 300.339° |
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Earth MOID | 0.793851 AU (118.7584 Gm) |
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Jupiter MOID | 2.55306 AU (381.932 Gm) |
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TJupiter | 3.605 |
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Synodic rotation period | 2.88 ± 0.12 h (0.120 ± 0.00500 d)[2] |
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Absolute magnitude (H) | 11.7 |
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Photometric observations of this asteroid in 2019 resulted in a light curve showing a rotation period of 2.721±0.003 h with a brightness variation of 0.06 in magnitude. This result is consistent with a similar study earlier in the year.[4] A. Kryszczynska and associates had found a slightly longer rotation period of 2.88 hours in 2012.[2] The low amplitude of the variation suggests a nearly spherical shape.[2] The spectrum of 711 Marmulla most closely matches an A-type asteroid.[5]
References
- "711 Marmulla (1911 LN)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- Kryszczynska, A.; et al. (October 2012). "Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region". Astronomy & Astrophysics. 546: 51. Bibcode:2012A&A...546A..72K. doi:10.1051/0004-6361/201219199. A72.
{{cite journal}}
: CS1 maint: postscript (link) - Schmadel, Lutz D. (2012), Dictionary of Minor Planet Names, Springer Berlin Heidelberg, p. 67, ISBN 9783642297182.
- Stephens, Robert D.; Warner, Brian D. (April 2020), "Main-Belt Asteroids Observed from CS3: 2019 October to December", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 47 (2): 125–133, Bibcode:2020MPBu...47..125S.
- Alvarez-Candal, A.; et al. (December 2006), "The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis", Astronomy and Astrophysics, 459 (3): 969–976, Bibcode:2006A&A...459..969A, doi:10.1051/0004-6361:20065518.
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На других языках
[de] (711) Marmulla
(711) Marmulla ist ein Asteroid des Hauptgürtels, der am 1. März 1911 vom österreichischen Astronomen Johann Palisa in Wien entdeckt wurde.
- [en] 711 Marmulla
[es] (711) Marmulla
711 Marmulla es un asteroide perteneciente a la familia Flora en el cinturón principal.[1] El nombre se deriva de la palabra del alto alemán antiguo 'marmul', que significa 'mármol'.
[ru] (711) Мармулла
(711) Мармулла (лат. Marmulla) — астероид из группы главного пояса, который входит в состав семейства Флоры[1]. Он был открыт 1 марта 1911 года австрийским астрономом Иоганном Пализой в Венской обсерватории и назван в честь мрамора (нем. Marmel)[2].
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