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1607 Mavis

From Wikipedia, the free encyclopedia
Stony asteroid

1607 Mavis
Lightcurve-based 3D-model ofMavis
Discovery[1]
Discovered byE. 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 · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc114.29 yr (41,743 days)
Aphelion3.3268AU
Perihelion1.7728 AU
2.5498 AU
Eccentricity0.3047
4.07yr (1,487 days)
158.86°
0° 14m 31.56s / day
Inclination8.5789°
122.53°
235.96°
Physical characteristics
Dimensions11.57±1.76 km[4]
12.10 km(derived)[3]
12.756±0.210 km[5][6]
14.91±0.25 km[7]
6.1339±0.0004h[8]
6.1508±0.0005 h[9]
0.189±0.007[7]
0.193±0.021[6]
0.2487±0.0428[5]
0.31±0.11[4]
0.3320(derived)[3]
S[3][10]
11.29±0.27[10] · 11.4[1][3] · 11.54[4] · 11.6[7][5]

1607 Mavis, provisional designation1950 RA, is a stonyasteroid from the central region of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 3 September 1950, by South African astronomerErnest Johnson atJohannesburg Observatory in South Africa.[11] It was later named Mavis Beacon.

Orbit and classification

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This asteroid orbits the Sun in themiddle main-belt at a distance of 1.8–3.3 AU once every 4 years and 1 month (1,487 days). Its orbit has aneccentricity of 0.30 and aninclination of 9° with respect to theecliptic.[1] The asteroid'sobservation arc begins with its official discovery observations, as the two previous identifications,A903 BH and1934 VQ, made atHeidelberg andSimeiz in 1903 and 1934, respectively, remained unused.[11]

Physical characteristics

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Mavis is a stonyS-type asteroid.[3][10]

Rotation period

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In September 2007, Australian astronomers Collin Bembrick and Julian Oey independently obtained two rotationallightcurves ofMavis. These well-defined lightcurves gave arotation period of 6.1339 and 6.1508 hours with a brightness variation of 0.50 and 0.53magnitude, respectively (U=3/3).[8][9]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Mavis measures between 11.57 and 14.91 kilometers in diameter and its surface has analbedo between 0.189 and 0.31.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.3320 and a diameter of 12.10 kilometers based on anabsolute magnitude of 11.4.[3]

Naming

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Thisminor planet was named in honor of the Mavis Bruwer, wife of astronomerJacobus Albertus Bruwer, who was an astronomer at Johannesburg Observatory, and after whom1811 Bruwer was named.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3931).[12]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1607 Mavis (1950 RA)" (2017-05-06 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1607) Mavis".Dictionary of Minor Planet Names – (1607) Mavis.Springer Berlin Heidelberg. p. 127.doi:10.1007/978-3-540-29925-7_1608.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1607) Mavis". Asteroid Lightcurve Database (LCDB). Retrieved29 December 2016.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^abcdMainzer, 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.S2CID 35447010.
  6. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved29 December 2016.
  7. ^abcdUsui, 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. (online,AcuA catalog p. 153)
  8. ^abBembrick, 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. Retrieved29 December 2016.
  9. ^abOey, 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. Retrieved29 December 2016.
  10. ^abcVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved29 December 2016.
  11. ^ab"1607 Mavis (1950 RA)".Minor Planet Center. Retrieved29 December 2016.
  12. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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