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1694 Kaiser

From Wikipedia, the free encyclopedia
Asteroid in the asteroid belt

1694 Kaiser
Shape model ofKaiser from itslightcurve
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
(Leiden Southern Station)
Discovery date29 September 1934
Designations
(1694) Kaiser
Named after
Frederik Kaiser(astronomer)[2]
1934 SB · 1960 SD
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.60 yr (30,168 days)
Aphelion3.0137AU
Perihelion1.7759 AU
2.3948 AU
Eccentricity0.2584
3.71yr (1,354 days)
125.25°
0° 15m 57.24s / day
Inclination11.103°
13.421°
356.15°
Physical characteristics
Dimensions13.84±1.27 km[4]
15.678±0.175 km[5][6]
28.42 km(calculated)[3]
9h[a]
13.02±0.01 h[7]
13.23±0.02 h[8]
0.057(assumed)[3]
0.1659±0.0088[5]
0.166±0.009[6]
0.241±0.046[4]
B–V = 0.735[1]
U–B = 0.415[1]
Tholen = GC[1] · C[3]
11.46[1][3][4][5]

1694 Kaiser (prov. designation:1934 SB) is a carbonaceousbackground asteroid from the inner regions of theasteroid belt, approximately 16 kilometers in diameter. It was discovered on 29 September 1934, by Dutch astronomerHendrik van Gent at Leiden Southern Station, annex to theJohannesburg Observatory in South Africa.[9] It is named for Dutch astronomerFrederik Kaiser.[2]

Orbit and classification

[edit]

Kaiser is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements. It orbits the Sun in theinner main-belt at a distance of 1.8–3.0 AU once every 3 years and 9 months (1,354 days). Its orbit has aneccentricity of 0.26 and aninclination of 11° with respect to theecliptic.of 1.8–3.0 AU once every 3.71 years (1,354 days). Itseccentric orbit of 0.26 isinclined by 11 degrees towards the plane of theecliptic.[1]Kaiser'sobservation arc begins with its official discovery observation, as noprecoveries were taken, and no prior identifications were made.[9]

Naming

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This asteroid was named in honor of Dutch astronomerFrederik Kaiser (1808–1872), the director of theLeiden Observatory from 1837 to 1872. He founded the new Leiden Observatory and stimulated Dutch astronomical research. Frederick Kaiser is also honored by thelunar andMartian cratersKaiser.[2] Originally, the asteroid was erroneously namedKapteyn (MPC 2822), and only later it was noticed that the Duch astronomerJacobus Kapteyn was already honored by the minor planet818 Kapteynia. The officialnaming citation was published by theMinor Planet Center on 15 July 1968 (M.P.C. 2883).[10]

Physical parameters

[edit]

Spectral type

[edit]

On theTholen taxonomy, the carbonaceousC-type asteroid is classified as a rare GC-type, an intermediate to theG-type asteroids.[1]

Diameter and albedo

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According to the survey the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Kaiser measures 13.84 and 15.68 kilometers in diameter, and its surface has analbedo of 0.241 and 0.166, respectively.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 28.42 kilometers, with anabsolute magnitude of 11.46[3]

Rotation period

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Two rotationallightcurves forKaiser were obtained from photometric observations by American astronomerBrian D. Warner at his Palmer Divide Observatory in Colorado(see video in§ External links). The lightcurves from January 2006 and November 2012, gave arotation period of 13.02 and 13.23 hours and a variation in brightness of 0.32 and 0.13magnitude, respectively (U=3/2+).[7][8]

Notes

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  1. ^CALL (2011web) gives a rotation period of 9 hours. Summary figures atLCDB Data for (1694) Kaiser

References

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  1. ^abcdefgh"JPL Small-Body Database Browser: 1694 Kaiser (1934 SB)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 December 2016. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1694) Kaiser".Dictionary of Minor Planet Names – (1694) Kaiser.Springer Berlin Heidelberg. p. 135.doi:10.1007/978-3-540-29925-7_1695.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1694) Kaiser". Asteroid Lightcurve Database (LCDB). Retrieved17 December 2016.
  4. ^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)
  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.
  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. Retrieved17 December 2016.
  7. ^abWarner, Brian D. (April 2013)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2012 September - 2013 January".The Minor Planet Bulletin.40 (2):71–80.Bibcode:2013MPBu...40...71W.ISSN 1052-8091. Retrieved17 December 2016.
  8. ^abWarner, Brian D. (September 2006)."Asteroid lightcurve analysis at the Palmer Divide Observatory - late 2005 and early 2006".The Minor Planet Bulletin.33 (3):58–62.Bibcode:2006MPBu...33...58W.ISSN 1052-8091. Retrieved17 December 2016.
  9. ^ab"1694 Kaiser (1934 SB)".Minor Planet Center. Retrieved17 December 2016.
  10. ^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]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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