Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1552 Bessel

From Wikipedia, the free encyclopedia
Main-belt asteroid

1552 Bessel
Shape model of Bessel from itslightcurve
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Observatory
Discovery date24 February 1938
Designations
(1552) Bessel
Named after
Friedrich Bessel
(German astronomer)[2]
1938 DE1 · 1933 FJ1
1948 EH · 1951 UF
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc84.11 yr (30,722 days)
Aphelion3.3068AU
Perihelion2.7174 AU
3.0121 AU
Eccentricity0.0978
5.23yr (1,909 days)
185.26°
0° 11m 18.6s / day
Inclination9.8367°
9.9835°
39.607°
Physical characteristics
Dimensions16.63±0.84 km[4]
18.33 km(derived)[3]
18.514±0.066 km[5]
18.817±0.101 km[6]
8.96318±0.00002 h[a]
8.996±0.006h[7]
0.1448(derived)[3]
0.1514±0.0332[6]
0.156±0.023[5]
0.193±0.024[4]
S[3]
11.3[4][6] · 11.4[1][3] · 11.53±0.24[8]

1552 Bessel (provisional designation1938 DE1) is a stony Eoanasteroid from the outer regions of theasteroid belt, approximately 18 kilometers in diameter. It was discovered on 24 February 1938, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland, and named after German astronomerFriedrich Bessel.[2][9]

Orbit and classification

[edit]

Bessel is astony asteroid and a member of theEos family that orbits the Sun in theouter main-belt at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,909 days). Its orbit has aneccentricity of 0.10 and aninclination of 10° with respect to theecliptic.[1] First observed as1933 FJ1 atHeidelberg in 1933, the body'sobservation arc begins at Turku, 5 days prior to its official discovery observation.[9]

Naming

[edit]

Thisminor planet was named after German astronomerFriedrich Wilhelm Bessel (1789–1846), who measured the firststellar parallax in 1838. His measured parallax of 0.314 arcseconds for61 Cygni gave a distance of 10.3 light-years, which is 9.6% off today's measured distance of 11.4 light-years. Bessel is also honored by the lunar craterBessel.[2][10] The officialnaming citation was published by theMinor Planet Center on 30 January 1964 (M.P.C. 2278).[11]

Physical characteristics

[edit]

Rotation period and pole

[edit]

In March 2011, a rotationallightcurve of Bessel was obtained from photometric observations by Italian amateur astronomerSilvano Casulli. Lightcurve analysis gave a well-definedrotation period of 8.996 hours with a brightness variation of 0.29magnitude (U=3).[7]

In 2016, a modeled lightcurve using photometric data from various sources gave a concurring period of 8.96318 hours, as well as aspin axis of (61.0°, −50.0°) inecliptic coordinates (λ, β).[a]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Bessel measures between 16.63 and 18.817 kilometers in diameter, and its surface has analbedo between 0.1514 and 0.193.[4][5][6] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1448 and a diameter of 18.33 kilometers with anabsolute magnitude of 11.4.[3]

Notes

[edit]
  1. ^abHanus (2016) web: rotation period of8.96318 hours. (λ, β)-Pole axis of (61.0°, −50.0°) and (221.0°, −57.0°) . Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1552) Bessel

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1552 Bessel (1938 DE1)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1552) Bessel".Dictionary of Minor Planet Names – (1552) Bessel.Springer Berlin Heidelberg. p. 123.doi:10.1007/978-3-540-29925-7_1553.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1552) Bessel". Asteroid Lightcurve Database (LCDB). Retrieved11 April 2017.
  4. ^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. Retrieved11 April 2017.
  5. ^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. Retrieved11 April 2017.
  6. ^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.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1552) Bessel".Geneva Observatory. Retrieved11 April 2017.
  8. ^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. Retrieved11 April 2017.
  9. ^ab"1552 Bessel (1938 DE1)".Minor Planet Center. Retrieved11 April 2017.
  10. ^"Friedrich Wilhelm Bessel (July 22, 1784 - March 17, 1846)". seds.org. Archived fromthe original on 4 February 2012. Retrieved11 April 2017.
  11. ^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.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
Retrieved from "https://en.wikipedia.org/w/index.php?title=1552_Bessel&oldid=1318736457"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp