Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

4949 Akasofu

From Wikipedia, the free encyclopedia
Main-belt asteroid

4949 Akasofu
Discovery[1]
Discovered byT. Kojima
Discovery siteYGCO Chiyoda Stn.
Discovery date29 November 1988
Designations
(4949) Akasofu
Named after
Syun-Ichi Akasofu
(geophysicist)[2]
1988 WE · 1978 YE
1981 RL5 · 1981 SV6
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.45 yr (14,044 days)
Aphelion2.6555AU
Perihelion1.8904 AU
2.2729 AU
Eccentricity0.1683
3.43yr (1,252 days)
163.34°
0° 17m 15.36s / day
Inclination4.8106°
108.70°
275.40°
Physical characteristics
Dimensions4.460±0.181 km[4][5]
5.67 km(calculated)[3]
2.6798±0.0002h[6]
2.6800±0.0003 h[a]
0.24(assumed)[3]
0.322±0.055[4][5]
S[3]
13.4[1][3] · 13.6[4] · 13.49±0.14[7]

4949 Akasofu, provisional designation1988 WE, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered by Japanese amateur astronomerTakuo Kojima at theYGCO Chiyoda Station in Japan on 29 November 1988.[8] The asteroid was named for Japanese geophysicistSyun-Ichi Akasofu

Orbit and classification

[edit]

Akasofu is a member of theFlora family, one of the largest groups ofstony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,252 days). Its orbit has aneccentricity of 0.17 and aninclination of 5° with respect to theecliptic.[1] In 1978, it was first identified as1978 YE at thePurple Mountain Observatory, extending the body'sobservation arc by 10 years prior to its official discovery observation at Chiyoda Station.[8]

Physical characteristics

[edit]

Rotation period

[edit]

According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Akasofu measures 4.5 kilometers in diameter and its surface has analbedo of 0.32,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – which derives from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 5.7 kilometers with anabsolute magnitude of 13.4.[3]

Diameter and albedo

[edit]

In October 2005, a rotationallightcurve ofAkasofu was obtained from photometric observations made by David Higgins at Hunters Hill Observatory, Australia. It showed arotation period of2.6798 hours with a brightness variation of 0.10 inmagnitude (U=3).[6]

Observations by Czech astronomerPetr Pravec in March 2007, gave another well-defined and concurring lightcurve with a period of2.6800 hours and an amplitude of 0.15 in magnitude (U=3).[a]

Naming

[edit]

Thisminor planet was named in honor of Japanese-born geophysicistSyun-Ichi Akasofu (born 1930), professor atUniversity of Alaska Fairbanks. He was the director of theInternational Arctic Research Center from 1998 to 2007, and is known for studies of theaurora borealis.[2] The official naming citation was published by theMinor Planet Center on 30 March 2010 (M.P.C. 69491).[9]

Notes

[edit]
  1. ^abPravec (2007):lightcuve plot for (4949) Akasofu, with a rotation period2.6800±0.0003 hours with a brightness amplitude of0.15 magnitude. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4949 Akasofu (1988 WE)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abSchmadel, Lutz D. (2003).Dictionary of Minor Planet Names – (4949) Akasofu.Springer Berlin Heidelberg. p. 402.ISBN 978-3-540-29925-7. Retrieved30 December 2015.
  3. ^abcdef"LCDB Data for (4949) Akasofu". Asteroid Lightcurve Database (LCDB). Retrieved3 May 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. Retrieved3 May 2016.
  5. ^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. Retrieved5 December 2016.
  6. ^abHiggins, David; Pravec, Petr; Kusnirak, Peter; Masi, Gianluca; Galad, Adrian; Gajdos, Stefan; et al. (March 2006)."Asteriod [sic] lightcurve analysis at Hunters Hill Observatory and collaborating stations - autumn/winter 2005".The Minor Planet Bulletin.33 (1):8–10.Bibcode:2006MPBu...33....8H.ISSN 1052-8091. Retrieved3 May 2016.
  7. ^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. Retrieved3 May 2016.
  8. ^ab"4949 Akasofu (1988 WE)".Minor Planet Center. Retrieved3 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2016.

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=4949_Akasofu&oldid=1313082876"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp