(311999) 2007 NS2
Discovery[1] | |
---|---|
Discovery site | Observatorio Astronómico de La Sagra |
Discovery date | 14 July 2007 |
Designations | |
Martian L5![]() | |
Orbital characteristics[2][3] | |
Epoch13 January 2016 (JD2457400.5) | |
Uncertainty parameter0 | |
Observation arc | 6296 days (17.24 yr) |
Aphelion | 1.6061055AU(240.26996Gm) |
Perihelion | 1.4414495 AU (215.63778 Gm) |
1.5237775 AU (227.95387 Gm) | |
Eccentricity | 0.0540289 |
1.88yr(687.04d) | |
29.476921° | |
0.5239885°/day | |
Inclination | 18.62037° |
282.49476° | |
176.94930° | |
Physical characteristics | |
Dimensions | 800–1600 m |
18.1 | |
(311999) 2007 NS2is anasteroidandMars trojanorbiting near theL5pointofMars.
Discovery, orbit and physical properties[edit]
(311999) 2007 NS2was discovered on 14 July 2007, by theObservatorio Astronómico de La Sagra.[4][5][6][7][8] Its orbit is characterized by low eccentricity (0.054), moderate inclination (18.6°) and a semi-major axis of 1.52 AU.[8]Upon discovery, it was classified asMars-crosserby theMinor Planet Center.Its orbit is well determined as it is currently (March 2013) based on 87 observations with a data-arc span of 4,800 days.[2]2007 NS2has an absolute magnitude of 17.8, which gives a characteristic diameter of 870 m.[2]
Mars trojan and orbital evolution[edit]
Jean Meeussuspected that(311999) 2007 NS2was a Mars Trojan, and this was confirmed by Reiner Stoss's analysis of two sets of observations dating from 1998 on the MPC database.[9]It was confirmed to be a Mars Trojan numerically in 2012.[10]Recent calculations confirm that it is a stableL5Mars Trojan asteroidwith a libration period of 1310 years and an amplitude of 14°.[11][12]These values as well as its short-term orbital evolution are similar to those of5261 Eureka.Out of all known Mars Trojans, it currently has the smallest relative (to Mars) semimajor axis, 0.000059 AU.[11]
Origin[edit]
Long-termnumerical integrationsshow that its orbit is very stable on Gyr time-scales (1 Gyr = 1 billion years). As in the case of Eureka, calculations in both directions of time (4.5 Gyr into the past and 4.5 Gyr into the future) indicate that(311999) 2007 NS2may be a primordial object, perhaps a survivor of the planetesimal population that formed in the terrestrial planets region early in the history of theSolar System.[11]
![](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d7/Animation_of_2007_NS2_relative_to_Sun_and_Mars_1600-2500.gif/220px-Animation_of_2007_NS2_relative_to_Sun_and_Mars_1600-2500.gif)
Sun·2007 NS2·Mars
See also[edit]
- 5261 Eureka(1990 MB)
- (101429) 1998 VF31
- (121514) 1999 UJ7
- (385250) 2001 DH47
- 2009 SE
- 2011 SC191
- 2011 SL25
- 2011 SP189
- 2011 UB256
- 2011 UN63
- 2016 CP31
- 2018 EC4
- 2018 FC4
- 2020 VT1
References[edit]
- ^"Major News About Minor Objects".16 July 2007. Archived fromthe originalon 6 August 2019.Retrieved22 April2009.
- ^abc"311999 (2007 NS2) orbit diagram".JPL Small-Body Database.Jet Propulsion Laboratory.SPK-ID:2311999.Retrieved28 March2016.
- ^AstDys-1
- ^2007 NS2 discovery blog
- ^Discovery MPEC
- ^Update MPEC
- ^New Scientist article on the discovery
- ^abMPC data on 2007 NS2
- ^"Table of contents".Britastro.org.Retrieved29 October2013.
- ^ Schwarz, R.; Dvorak, R. (2012). "Trojan capture by terrestrial planets".Celestial Mechanics and Dynamical Astronomy.113(1): 23.arXiv:1611.07413.Bibcode:2012CeMDA.113...23S.doi:10.1007/s10569-012-9404-4.S2CID254375599.
- ^abc de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (2013)."Three new stable L5 Mars Trojans".Monthly Notices of the Royal Astronomical Society Letters.432(1): L31–L35.arXiv:1303.0124.Bibcode:2013MNRAS.432L..31D.doi:10.1093/mnrasl/slt028.
- ^ Christou, A. A. (2013). "Orbital clustering of Martian Trojans: An asteroid family in the inner solar system?".Icarus.224(1): 144–153.arXiv:1303.0420.Bibcode:2013Icar..224..144C.doi:10.1016/j.icarus.2013.02.013.S2CID119186791.
Further reading[edit]
- Rodriguez, J.; et al. (2007). "2007 NS2".Minor Planet Electronic Circular.2007-O03: 2007–0303.Bibcode:2007MPEC....O...03R.
- Skiff, B. A.; et al. (2007). "2007 NS2".Minor Planet Electronic Circular.2007-O09: 2007–O09.Bibcode:2007MPEC....O...09S.
- Schwarz, R.; Dvorak, R. (2007). "Trojan capture by terrestrial planets".Celestial Mechanics and Dynamical Astronomy.113(1): 23.arXiv:1611.07413.Bibcode:2012CeMDA.113...23S.doi:10.1007/s10569-012-9404-4.S2CID254375599.
- de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (2013)."Three new stable L5 Mars Trojans".Monthly Notices of the Royal Astronomical Society Letters.432(1): L31.arXiv:1303.0124.Bibcode:2013MNRAS.432L..31D.doi:10.1093/mnrasl/slt028.
- Christou, A. A. (2007). "Orbital clustering of martian Trojans: An asteroid family in the inner Solar System?".Icarus.224(1): 144.arXiv:1303.0420.Bibcode:2013Icar..224..144C.doi:10.1016/j.icarus.2013.02.013.S2CID119186791.
External links[edit]
- 2007 NS2data at MPC.
- (311999) 2007 NS2atAstDyS-2, Asteroids—Dynamic Site
- (311999) 2007 NS2at theJPL Small-Body Database