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1043 Beate

From Wikipedia, the free encyclopedia
Stony asteroid

1043 Beate
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date22 April 1925
Designations
(1043) Beate
PronunciationGerman:[beːˈʔaːtə][2]
Named after
unknown[3]
1925 HB
main-belt · (outer)[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc92.20 yr (33,677 days)
Aphelion3.2214AU
Perihelion2.9717 AU
3.0966 AU
Eccentricity0.0403
5.45yr (1,990 days)
255.00°
0° 10m 51.24s / day
Inclination8.9257°
159.31°
154.71°
Physical characteristics
Dimensions31.60±1.3 km[5]
31.85 km(derived)[4]
31.986±0.075 km[6]
33.97±0.43 km[7]
34.08±1.11 km[8]
40.952±0.967 km[9]
14.6±0.1 h[10]
44.3±0.1h[11][a]
0.1283±0.0193[9]
0.188±0.006[7]
0.209±0.032[6]
0.2147±0.019[5]
0.241±0.038[8]
0.2517(derived)[4]
Tholen =S[1] · S[4]
B–V = 0.900[1]
U–B = 0.455[1]
9.50[8] · 9.6[1][4] · 9.79[5][7][9] · 9.90±0.21[12]

1043 Beate, provisional designation1925 HB, is a stonyasteroid from the outer region of theasteroid belt, approximately 32 kilometers in diameter. It was discovered by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory on 22 April 1925.[13] Any reference of its name to a person is unknown.[3]

Orbit and classification

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Beate orbits the Sun in theouter main-belt at a distance of 3.0–3.2 AU once every 5 years and 5 months (1,990 days). Its orbit has aneccentricity of 0.04 and aninclination of 9° with respect to theecliptic.[1] The asteroid'sobservation arc begins at the discovering observatory in May 1925, 3 weeks after its official discovery observation.[13]

Physical characteristics

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In theTholen classification,Beate is a commonS-type asteroid.[1]

Rotation period

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In April 2006, a rotationallightcurve ofBeate was obtained from photometric observations by American astronomerBrian Warner at his Palmer Divide Observatory (716) in Colorado. It gave a longer-than averagerotation period of44.3±0.1 hours with a brightness variation of 0.47magnitude (U=2+).[11][a]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Beate measures between 31.6 and 41.0 kilometers in diameter and its surface has analbedo between 0.128 and 0.241.[5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2517 and a diameter of 31.85 kilometers with anabsolute magnitude of 9.6.[4]

Naming

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For thisminor planet, any reference of its name to a person or occurrence is unknown.[3]

Unknown meaning

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Among the many thousands ofnamed minor planets,Beate is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between164 Eva and1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomersAuguste Charlois,Johann Palisa,Max Wolf andKarl Reinmuth.[14]

Notes

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  1. ^abLightcurve plot of 1043 Beate, Palmer Divide Observatory, Brian D. Warner (2006)

References

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  1. ^abcdefgh"JPL Small-Body Database Browser: 1043 Beate (1925 HB)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 22 December 2019. Retrieved26 July 2017.
  2. ^(German Names)
  3. ^abcSchmadel, Lutz D. (2007). "(1043) Beate".Dictionary of Minor Planet Names – (1043) Beate.Springer Berlin Heidelberg. p. 89.doi:10.1007/978-3-540-29925-7_1044.ISBN 978-3-540-00238-3.
  4. ^abcdef"LCDB Data for (1043) Beate". Asteroid Lightcurve Database (LCDB). Retrieved8 November 2016.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  6. ^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. Retrieved6 November 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. ^abcdMasiero, 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. Retrieved8 November 2016.
  9. ^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.
  10. ^Behrend, Raoul."Asteroids and comets rotation curves – (1043) Beate".Geneva Observatory. Retrieved8 November 2016.
  11. ^abWarner, Brian D.; Higgins, David (December 2006)."The lightcurves of 1043 Beate and 1186 Turnera".The Minor Planet Bulletin.33 (4):104–105.Bibcode:2006MPBu...33..104W.ISSN 1052-8091. Retrieved8 November 2016.
  12. ^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. Retrieved8 November 2016.
  13. ^ab"1043 Beate (1925 HB)".Minor Planet Center. Retrieved8 November 2016.
  14. ^Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning".Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929.ISBN 978-3-540-00238-3.

External links

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