Astronomy:2009 SE
Discovery | |
---|---|
Discovered by | Catalina Sky Survey |
Discovery date | 16 September 2009 |
Designations | |
2009 SE | |
Minor planet category | Martian L5 |
Orbital characteristics[1] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 0 | |
Observation arc | 3133 days (8.58 yr) |
|{{{apsis}}}|helion}} | 1.623684 astronomical unit|AU (242.8997 Gm) |
|{{{apsis}}}|helion}} | 1.425261 AU (213.2160 Gm) |
1.524472 AU (228.0578 Gm) | |
Eccentricity | 0.0650794 |
Orbital period | 1.88 yr (687.508 d) |
Mean anomaly | 240.916° |
Mean motion | 0° 31m 25.069s /day |
Inclination | 20.6248° |
Longitude of ascending node | 6.82030° |
354.156° | |
Earth MOID | 0.42422 AU (63.462 Gm) |
Jupiter MOID | 3.5304 AU (528.14 Gm) |
Physical characteristics | |
Mean diameter | 400 m |
Geometric albedo | 0.5–0.05 (assumed) |
Absolute magnitude (H) | 19.9 |
2009 SE is a small asteroid and Mars trojan orbiting near the L5 point of Mars (60 degrees behind Mars on its orbit).[2]
Discovery, orbit and physical properties
2009 SE was first observed on 16 September 2009 by the Catalina Sky Survey (CSS).[3] Its orbit is characterized by low eccentricity (0.065), moderate inclination (20.6°) and a semi-major axis of 1.52 AU.[3] Upon discovery, it was classified as Mars-crosser by the Minor Planet Center. Its orbit is well determined as it is currently (January 2021) based on 56 observations with a data-arc span of 3,133 days.[1] 2009 SE has an absolute magnitude of 19.9 which gives a characteristic diameter of 400 m.[1]
Mars trojan and orbital evolution
Recent calculations indicate that it is a stable L5 Mars trojan with a libration period of 1430 yr and an amplitude of 70°.[2] The libration amplitude is not similar to that of 5261 Eureka and related objects.[citation needed]
Mars trojan
L4 (leading):
L5 (trailing):
- 5261 Eureka (1990 MB) †
- (101429) 1998 VF31 †
- (311999) 2007 NS2 †
- (385250) 2001 DH47
- 2009 SE
- 2011 SC191
- 2011 SL25
- 2011 SP189
- 2011 UB256
- 2011 UN63
- 2016 CP31
- 2018 EC4
- 2018 FC4
See also
References
- ↑ 1.0 1.1 1.2 "JPL Small-Body Database Browser: (2009 SE)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2009SE;cad=1.
- ↑ 2.0 2.1 de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (March 2021). "Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space". Monthly Notices of the Royal Astronomical Society 501 (4): 6007–6025. doi:10.1093/mnras/stab062. Bibcode: 2021MNRAS.501.6007D. https://academic.oup.com/mnras/article-abstract/501/4/6007/6081058.
- ↑ 3.0 3.1 MPC data on 2009 SE
Further reading
- Three new stable L5 Mars Trojans de la Fuente Marcos, C., de la Fuente Marcos, R. 2013, Monthly Notices of the Royal Astronomical Society: Letters, Vol. 432, Issue 1, pp. 31–35.
- Orbital clustering of Martian Trojans: An asteroid family in the inner solar system? Christou, A. A. 2013, Icarus, Vol. 224, Issue 1, pp. 144–153.
External links
Original source: https://en.wikipedia.org/wiki/2009 SE.
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