Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1209 Pumma

From Wikipedia, the free encyclopedia
Hygiean asteroid discovered in 1927

1209 Pumma
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date22 April 1927
Designations
(1209) Pumma
Named after
Niece of discoverer's friend[2]
1927 HA · 1950 JQ
1963 UU
main-belt · (outer)[3]
Hygiea[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc90.20 yr (32,945 days)
Aphelion3.5836AU
Perihelion2.7590 AU
3.1713 AU
Eccentricity0.1300
5.65yr (2,063 days)
302.93°
0° 10m 28.2s / day
Inclination6.9333°
89.806°
176.87°
Physical characteristics
Dimensions21.73±2.15 km[5]
26.889±0.253 km[6]
26.986±0.311 km[7]
40.33 km (calculated)[3]
8.5001±0.0001h[8]
0.057 (assumed)[3]
0.1397±0.0360[7]
0.141±0.028[6]
0.215±0.055[5]
C (assumed)[3]
10.60[5][7] · 10.62±0.19[9] · 10.7[1][3]

1209 Pumma (provisional designation1927 HA) is aHygieanasteroid from the outer region of theasteroid belt, approximately 30 kilometers in diameter. It was discovered on 22 April 1927, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[10] The asteroid was named after the niece of astronomerAlbrecht Kahrstedt.[2]

Orbit and classification

[edit]

Pumma is a member of theHygiea family (601),[4] a very largefamily of carbonaceous outer-belt asteroids, named after thefourth-largest asteroid,10 Hygiea.[11] It orbits the Sun in theouter main-belt at a distance of 2.8–3.6 AU once every 5 years and 8 months (2,063 days). Its orbit has aneccentricity of 0.13 and aninclination of 7° with respect to theecliptic.[1] Noprecoveries were taken, and no prior identifications were made. The body'sobservation arc begins atUccle, 8 days after its official discovery observation at Heidelberg.[10]

Physical characteristics

[edit]

Lightcurve

[edit]

In April 2012, a rotationallightcurve of Pumma was obtained from photometric observations by Italian and French amateur astronomersSilvano Casulli andRené Roy. Lightcurve analysis gave a well-definedrotation period of 8.5001 hours with a brightness variation of 0.28magnitude (U=3).[8]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Pumma measures between 21.73 and 26.99 kilometers in diameter, and its surface has analbedo between 0.139 and 0.215.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceousC-type asteroids of 0.057 and consequently calculates a much larger diameter of 40.33 kilometers using anabsolute magnitude of 10.7.[3]

Naming

[edit]

Thisminor planet's name was proposed by German astronomer Albrecht Kahrstedt (1897–1971), a staff member atARI and later director atBabelsberg Observatory(also see1587 Kahrstedt). "Pumma" is the nickname of a niece of Kahrstedt.[2][12][13] The official naming citation was published byPaul Herget inThe Names of the Minor Planets in 1955 (H 112).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1209 Pumma (1927 HA)" (2017-07-03 last obs.).Jet Propulsion Laboratory. Retrieved26 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1209) Pumma".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 101.doi:10.1007/978-3-540-29925-7_1210.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1209) Pumma". Asteroid Lightcurve Database (LCDB). Retrieved27 January 2017.
  4. ^ab"Asteroid 1209 Pumma – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  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. Retrieved27 January 2017.
  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. Retrieved27 January 2017.
  7. ^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.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1209) Pumma".Geneva Observatory. Retrieved27 January 2017.
  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.S2CID 53493339. Retrieved27 January 2017.
  10. ^ab"1209 Pumma (1927 HA)".Minor Planet Center. Retrieved27 January 2017.
  11. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  12. ^"1587 Kahrstedt (1933 FS1)".Minor Planet Center. Retrieved27 January 2017.
  13. ^Kahrstedt, Albrecht. Astronom, * 24.8.1897 Neiße (Oberschlesien), † 1.11.1971 Berlin (evangelisch) (in German). 1977. Retrieved22 November 2015.{{cite book}}:|work= ignored (help)

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=1209_Pumma&oldid=1217452539"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp