Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1844 Susilva

From Wikipedia, the free encyclopedia
Stony Eoan asteroid

1844 Susilva
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date30 October 1972
Designations
(1844) Susilva
Named after
Susi Petit–Pierre
(friend of discoverer)[2]
1972 UB · 1943 EU
1953 AA · 1959 GJ
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.40 yr (23,521 days)
Aphelion3.1714AU
Perihelion2.8587 AU
3.0150 AU
Eccentricity0.0518
5.24yr (1,912 days)
70.711°
0° 11m 17.88s / day
Inclination11.788°
99.365°
73.564°
Physical characteristics
Dimensions19.022±0.232 km[4]
22.41 km(calculated)[3]
26.800±0.321 km[5]
0.118±0.011[5]
0.14(assumed)[3]
0.2358±0.0545[4]
S[3]
10.8[4][5] · 11.0[1][3] · 11.49±0.44[6]

1844 Susilva, provisional designation1972 UB, is a stony Eoanasteroid from the outer region of theasteroid belt, approximately 22 kilometers in diameter. It was discovered on 30 October 1972, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland, and later named after a schoolfriend of the discoverer.[2][7]

Classification and orbit

[edit]

Susilva is a member of theEos family, a collisional group of more than 4,000 asteroids, which are well known for mostly being ofsilicaceous composition. It orbits the Sun in theouter main-belt at a distance of 2.9–3.2 AU once every 5 years and 3 months (1,912 days). Its orbit has aneccentricity of 0.05 and aninclination of 12° with respect to theecliptic.[1]First identified as1943 EU atTurku Observatory,Susilva's first used observation was taken atUccle Observatory in 1953, extending the body'sobservation arc by 19 years prior to its official discovery observation.[7]

Physical characteristics

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures between 19.0 and 26.8 kilometers in diameter, and its surface has analbedo of 0.118 to 0.236.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.14, taken from221 Eos, the family's largest member and namesake – and calculates a diameter of 22.4 kilometers based on an absolutemagnitude of 11.0.[3]Susilva'srotation period has not yet been measured.[3]

Naming

[edit]

The discoverer named a pair of asteroids after two of his former schoolmates, Susi and Helen, both from the small village ofWald, Zürich in Switzerland. This one was dedicated to Susi Petit–Pierre, while the subsequently numbered asteroid,1845 Helewalda, was given to Helen Gachnang.[2][8] The officialnaming citation was published by theMinor Planet Center on 18 April 1977 (M.P.C. 4156).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1844 Susilva (1972 UB)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1844) Susilva".Dictionary of Minor Planet Names – (1844) Susilva.Springer Berlin Heidelberg. p. 148.doi:10.1007/978-3-540-29925-7_1845.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1844) Susilva". Asteroid Lightcurve Database (LCDB). Retrieved1 March 2016.
  4. ^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. Retrieved1 March 2016.
  5. ^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. Retrieved1 March 2016.
  6. ^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. Retrieved1 March 2016.
  7. ^ab"1844 Susilva (1972 UB)".Minor Planet Center. Retrieved1 March 2016.
  8. ^"Himmlischer Besuch auf der Sternwarte Eschenberg" (in German). Sternwarte Eschenberg. Retrieved1 March 2016.Helen Gachnang and Susi Petit-Pierre visit the Eschenberg Observatory
  9. ^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
Retrieved from "https://en.wikipedia.org/w/index.php?title=1844_Susilva&oldid=1273323050"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp