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(5407) 1992 AX
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Mars-crossing asteroid binary
November 2018
yes
(5407) 1992 AX
#FA8072
File:Orbit of 1992 AX.gif
Orbital diagram of 1992 AX
S. UedaH. Kaneda
Kushiro Obs.
4 January 1992
(5407) 1992 AX
1987 BH 2
Mars crosserbinary
27 April 2019 (JD 2458600.5)
0
66.90 yr (24,434 d)
2.3486 AU
1.3279 AU
1.8383 AU
0.2776
2.49 yr (910 d)
263.87°
0.3955 ms / day
11.390°
117.74°
108.78°
0.377 AU (147 LD)
1 (D: 780 m; P: 13.52 h)
2.78 0.55 km3.60 0.36 km3.8 0.4 km4.18 0.12 km
2.5488 h
0.1990.2940.3760.40
SMASS SkSB–V 0.690V–R 0.500V–I 0.840
13.9014.014.47
(5407) 1992 AX is a stony asteroid and a synchronous binary Mars-crosser from the innermost region of the asteroid belt, approximately 3.6 km mi off 2 us in diameter. It was discovered on 4 January 1992, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at the Kushiro Observatory on Hokkaidō, Japan. The S-type asteroid has a short rotation period of 2.5 hours. Its sub-kilometer satellite was discovered in 1997. As of 2018, the binary system has not been named.
Orbit and classification
1992 AX is a member of the Mars-crossing asteroids, a dynamically unstable group between the main belt and the near-Earth populations, crossing the orbit of Mars at 1.66 AU. It orbits the Sun at a distance of 1.3–2.3 AU once every 2 years and 6 months (910 days; semi-major axis of 1.84 AU). Its orbit has an eccentricity of 0.28 and an inclination of 11° with respect to the ecliptic.
The asteroid makes occasional close approaches to Mars. Its next close approach, on 22 January 2027, will bring it 0.0753 AU km on flip from Mars. The body's observation arc begins with a precovery taken at Palomar Observatory in November 1951, or more than 40 years prior to its official discovery observation at Kushiro.
Naming
This minor planet was numbered by the Minor Planet Center on 9 December 1992 (M.P.C. 21249). As of 2018, it has not been named.
Physical characteristics
1992 AX has been characterized as a common, stony S-type asteroid. In the SMASS taxonomy, it is an Sk-subtype, that transitions between the S and K-type asteroids. The body's color indices of 0.690 (B–V), 0.500 (V–R) and 0.840 (V–I) were also determined.
Lightcurves
Rotation period
Since 1997, several rotational lightcurves of 1992 AX have been obtained from photometric observations by Petr Pravec and collaborating astronomers. Best-rated lightcurve analysis gave a rotation period of 2.5488 hours with a consolidated brightness amplitude between 0.10 and 0.12 magnitude (U=2/3). The results supersedes a tentative period determination of 3.6 hours by Marc Buie (U=1).
Satellite
During the observations in January 1997, it was also revealed that 1992 AX is a synchronous binary asteroid with a minor-planet moon in its orbit. The satellite measures approximately 780 meters in diameter, or about 20% of its primary, and has an orbital period of 13.52 hours with an estimated semi-major axis of 5.8 kilometers for its very circular orbit. Observations by Pravec in January and February 2012 confirmed the binary nature of this asteroid, as well as its rotational and orbital periods.
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite, the Spitzer Space Telescope and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), 1992 AX measures between 2.78 and 4.18 kilometers in diameter and its surface has an albedo between 0.199 and 0.40.
In 2017, a study by WISE dedicated to Mars-crossing asteroids determined a diameter of 3.60 kilometers with a high albedo of 0.376. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and derives a diameter of 3.79 kilometers based on an absolute magnitude of 14.47. The Johnston's archive gives an effective (combined) diameter of 3.98 kilometers with 3.9 and 0.78 kilometers for its primary and secondary body, respectively.
References
30em 2018-10-21 last obs.
JPL Small-Body Database Browser: 5407 (1992 AX)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2005407;cad=1
Jet Propulsion Laboratory
19 November 2018
5407 (1992 AX)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=5407
19 November 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
19 November 2018
Asteroid (5407) 1992 AX
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=5407
19 November 2018
Asteroids with Satellites Database – (450894) 2008 BT18
Johnston's Archive
Johnston Wm. Robert
18 February 2017
http://www.johnstonsarchive.net/astro/astmoons/am-05407.html
19 November 2018
5407
19 November 2018
6
Fumihiko Usui
Daisuke Kuroda
Thomas G. Müller
Sunao Hasegawa
Masateru Ishiguro
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Shinki Oyabu
Munetaka Ueno
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Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
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2012Icar..221.1130M
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161887
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Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data
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119224590
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NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos
The Astronomical Journal
152
3
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Petr Pravec
Lenka Sarounová
David L. Rabinowitz
Michael D. Hicks
Marek Wolf
Yurij N. Krugly
Fiodor P. Velichko
Vasilij G. Shevchenko
Vasilij G. Chiorny
Ninel M. Gaftonyuk
Guy Genevier
July 2000
Two-Period Lightcurves of 1996 FG 3, 1998 PG, and (5407) 1992 AX: One Probable and Two Possible Binary Asteroids
Icarus
146
1
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2000Icar..146..190P
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6
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G. Esquerdo
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E. S. Howell
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Yu. N. Krugly
D. Tholen
R. Whiteley
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A. Grauer
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V. Reddy
S. Moore
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G. Masi
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G. Funkhouser
B. Knight
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M. Grenon
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C. Demeautis
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External links
Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
5407
5406 Jonjoseph 5407 5408 Thé
005407
Category:Discoveries by Hiroshi Kaneda
Category:Discoveries by Seiji Ueda
005407
005407
19920104