Jump to content

1607 Mavis

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by JJMC89 bot (talk | contribs) at 05:14, 23 September 2016 (Remove {{JPL small body}} parameter(s) migrated to Wikidata per request) (AWB (12089)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

1607 Mavis
Light-curve-based 3D-model of 1607 Mavis
Discovery [1]
Discovered byErnest Johnson
Discovery siteJohannesburg Obs.
Discovery date3 September 1950
Designations
1607 Mavis
Named after
Mavis Bruwer
(wife of astronomer)
Jacobus Bruwer[2]
1950 RA · 1934 VQ
1958 OB · 1958 PD
A903 BH
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc113.04 yr (41288 days)
Aphelion3.3277 AU (497.82 Gm)
Perihelion1.7715 AU (265.01 Gm)
2.5496 AU (381.41 Gm)
Eccentricity0.30520
4.07 yr (1487.0 d)
13.552°
0° 14m 31.56s / day
Inclination8.5808°
122.54°
235.95°
Earth MOID0.781794 AU (116.9547 Gm)
Jupiter MOID2.15174 AU (321.896 Gm)
TJupiter3.359
Physical characteristics
Dimensions11.97 km
14.91±0.25 km[4]
12.756±0.210 km[5]
12.18 km (derived)[3]
5.985 ± 0.5 km
6.1339 h (0.25558 d)[1][6]
6.1508±0.0005 h[7]
0.2826
0.189±0.007[4]
0.2487±0.0428[5]
0.3598 (derived)[3]
0.2826 ± 0.052[1]
S[3]
11.4

1607 Mavis, provisional designation 1950 RA, is an eccentric, stony asteroid from the inner regions of the asteroid belt, about 12 kilometers in diameter. It was discovered by South African astronomer Ernest Johnson at Union Observatory in Johannesburg on 3 September 1950.[8]

The asteroid orbits the Sun at a distance of 1.8–3.3 AU once every 4 years and 1 month (1,487 days). Its orbit shows an eccentricity of 0.31 and is tilted by 9 degrees to the plane of the ecliptic. It has a rotation period of 6.1 hours.[6][7] The stony S-type asteroid's albedo has been determined by the Akari and WISE missions to amount to 0.189±0.007 and 0.2487±0.0428, respectively, while the Lightcurve Database project derived a much higher value of 0.36.[3]

It was named in honor of the Mavis Bruwer, wife of astronomer Jacobus Albertus Bruwer, astronomer at the observatory in Johannesburg, after whom the minor planet 1811 Bruwer was named.[2]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1607 Mavis (1950 RA)" (2015-10-16 last obs.). Jet Propulsion Laboratory. Retrieved 25 April 2016.
  2. ^ a b Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1607) Mavis. Springer Berlin Heidelberg. p. 127. ISBN 978-3-540-29925-7. Retrieved 15 November 2015.
  3. ^ a b c d e "LCDB Data for (1607) Mavis". Asteroid Lightcurve Database (LCDB). Retrieved 15 November 2015.
  4. ^ a b Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 15 November 2015.
  5. ^ a b Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 15 November 2015.
  6. ^ a b Bembrick, Collin; Allen, Bill; Bolt, Greg (June 2008). "The Rotation Periods of 845 Naema, 1607 Mavis, and (30105) 2000 FO3". The Minor Planet Bulletin. 35 (2): 74–75. Bibcode:2008MPBu...35...74B. ISSN 1052-8091. Retrieved 15 November 2015.
  7. ^ a b Oey, Julian (September 2008). "Lightcurve Analysis of Asteroids from the Kingsgrove and Leura Observatories in the 2nd Half of 2007". The Minor Planet Bulletin. 35 (3): 132–135. Bibcode:2008MPBu...35..132O. ISSN 1052-8091. Retrieved 15 November 2015.
  8. ^ "1607 Mavis (1950 RA)". Minor Planet Center. Retrieved 15 November 2015.