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1658 Innes

From Wikipedia, the free encyclopedia
Main-belt asteroid

1658 Innes
Discovery[1]
Discovered byJ. A. Bruwer
Discovery siteJohannesburg Obs.
Discovery date13 July 1953
Designations
(1658) Innes
Named after
Robert T. A. Innes
(astronomer)[2]
1953 NA · 1940 GB
1948 EM · 1949 QA
1953 OF · 1953 PN
1957 OE
main-belt · (middle)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc77.08 yr (28,155 days)
Aphelion3.0302AU
Perihelion2.0866 AU
2.5584 AU
Eccentricity0.1844
4.09yr (1,495 days)
247.27°
0° 14m 27.24s / day
Inclination9.0941°
95.441°
188.76°
Physical characteristics
Dimensions13.352±0.140 km[3]
13.54±1.17 km[4]
14.082±0.042 km[5]
14.76 km(calculated)[6]
3.191±0.001h[7][8]
0.20(assumed)[6]
0.2241±0.0369[5]
0.248±0.019[3]
0.626±0.318[4]
B–V = 0.960[1]
U–B = 0.610[1]
Tholen = AS[1] · AS[6]
11.27±0.41[9] · 10.47[4] · 11.52[1][6][5]

1658 Innes, provisional designation1953 NA, is a rare-typeasteroid from the middle region of theasteroid belt, approximately 15 kilometers in diameter. It was named afterRobert T. A. Innes.

Discovery

[edit]

Innes was discovered on 13 July 1953, by South African astronomerJacobus Bruwer atJohannesburg Observatory in South Africa.[10]

It was the first numbered discovery of astronomer Jacobus Bruwer. In addition, he also discovered the minor planets1660 Wood,1794 Finsen, and3284 Niebuhr. The asteroid1811 Bruwer was named in his honour by the Dutch, Dutch-American astronomer trio of thePalomar–Leiden survey.[11]

Orbit and classification

[edit]

It orbits the Sun in thecentral main-belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,495 days). Its orbit has aneccentricity of 0.18 and aninclination of 9° with respect to theecliptic.[1]Innes was first identified as1940 GB atTurku Observatory in 1940, extending the body'sobservation arc by 13 years prior to its official discovery observation.[10]

Physical characteristics

[edit]

In theTholen taxonomy,Innes has an AS-spectral type, an intermediate form of the rareA-types to the commonstony asteroids(also seecategory listing).[12]

Rotation period

[edit]

In May 2005, astronomersRobert Stephens at the Center for Solar System Studies, California, and Lorenzo Franco at Balzaretto Observatory, near Rome, each obtained a rotationallightcurve ofInnes. The photometric observations gave an identicalrotation period of3.191±0.001 hours with a brightness variation of 0.22 and 0.25magnitude, respectively (U=3/3).[7][8]

Diameter and albedo

[edit]

According to the 2014-revised survey result of NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Innes measures 13.35 kilometers in diameter and its surface has analbedo of 0.248,[3] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 14.76 kilometers with anabsolute magnitude of 11.52.[6]

Naming

[edit]

Thisminor planet was named for Scottish–South African astronomerRobert T. A. Innes (1861–1933), first director of the discovering Union Observatory from 1903 to 1927 (originally named Transvaal Observatory). He was a skilledobservational astronomer, famous for his deliberate search for and discovery of the nearest star,Proxima Centauri, in 1915. He also made important theoretical and computational contributions tocelestial mechanics and to the irregularrotation of the Earth. The astronomer is also honored by the lunar craterInnes.[2] The officialnaming citation was published by theMinor Planet Center on 1 July 1972 (M.P.C. 3297).[13]

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 1658 Innes (1953 NA)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1658) Innes".Dictionary of Minor Planet Names – (1658) Innes.Springer Berlin Heidelberg. p. 132.doi:10.1007/978-3-540-29925-7_1659.ISBN 978-3-540-00238-3.
  3. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved23 December 2016.
  4. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved23 December 2016.
  5. ^abcMainzer, 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.
  6. ^abcde"LCDB Data for (1658) Innes". Asteroid Lightcurve Database (LCDB). Retrieved23 December 2016.
  7. ^abFranco, Lorenzo; Papini, Riccardo (October 2014)."Rotational Period for 1658 Innes, (10597) 1995 TR10, and 30017 Shaundatta".The Minor Planet Bulletin.41 (4):243–244.Bibcode:2014MPBu...41..243F.ISSN 1052-8091. Retrieved23 December 2016.
  8. ^abStephens, Robert D. (October 2014)."Asteroids Observed from CS3: 2014 April-June".The Minor Planet Bulletin.41 (4):226–230.Bibcode:2014MPBu...41..226S.ISSN 1052-8091. Retrieved23 December 2016.
  9. ^Veres, 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. Retrieved23 December 2016.
  10. ^ab"1658 Innes (1953 NA)".Minor Planet Center. Retrieved23 December 2016.
  11. ^Schmadel, Lutz D. (2007). "(1811) Bruwer".Dictionary of Minor Planet Names – (1811) Bruwer. Springer Berlin Heidelberg. p. 145.doi:10.1007/978-3-540-29925-7_1812.ISBN 978-3-540-00238-3.
  12. ^"JPL Small-Body Database Search Engine: spec. type = A (SMASSII)". JPL Solar System Dynamics. Retrieved23 December 2016.
  13. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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