Astronomy:4949 Akasofu

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4949 Akasofu
Discovery [1]
Discovered byT. Kojima
Discovery siteYGCO Chiyoda Stn.
Discovery date29 November 1988
Designations
(4949) Akasofu
Named afterSyun-Ichi Akasofu
(geophysicist)[2]
1988 WE · 1978 YE
1981 RL5 · 1981 SV6
Minor planet categorymain-belt · Flora [3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.45 yr (14,044 days)
|{{{apsis}}}|helion}}2.6555 AU
|{{{apsis}}}|helion}}1.8904 AU
2.2729 AU
Eccentricity0.1683
Orbital period3.43 yr (1,252 days)
Mean anomaly163.34°
Mean motion0° 17m 15.36s / day
Inclination4.8106°
Longitude of ascending node108.70°
275.40°
Physical characteristics
Dimensions4.460±0.181 km[4][5]
5.67 km (calculated)[3]
Rotation period2.6798±0.0002 h[6]
2.6800±0.0003 h[lower-alpha 1]
Geometric albedo0.24 (assumed)[3]
0.322±0.055[4][5]
S [3]
Absolute magnitude (H)13.4[1][3] · 13.6[4] · 13.49±0.14[7]


4949 Akasofu, provisional designation 1988 WE, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered by Japanese amateur astronomer Takuo Kojima at the YGCO Chiyoda Station in Japan on 29 November 1988.[8] The asteroid was named for Japanese geophysicist Syun-Ichi Akasofu

Orbit and classification

Akasofu is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,252 days). Its orbit has an eccentricity of 0.17 and an inclination of 5° with respect to the ecliptic.[1] In 1978, it was first identified as 1978 YE at the Purple Mountain Observatory, extending the body's observation arc by 10 years prior to its official discovery observation at Chiyoda Station.[8]

Physical characteristics

Rotation period

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Akasofu measures 4.5 kilometers in diameter and its surface has an albedo of 0.32,[4][5] while the Collaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – which derives from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 5.7 kilometers with an absolute magnitude of 13.4.[3]

Diameter and albedo

In October 2005, a rotational lightcurve of Akasofu was obtained from photometric observations made by David Higgins at Hunters Hill Observatory, Australia. It showed a rotation period of 2.6798 hours with a brightness variation of 0.10 in magnitude ({{{1}}}).[6]

Observations by Czech astronomer Petr Pravec in March 2007, gave another well-defined and concurring lightcurve with a period of 2.6800 hours and an amplitude of 0.15 in magnitude ({{{1}}}).[lower-alpha 1]

Naming

This minor planet was named in honor of Japanese-born geophysicist Syun-Ichi Akasofu (born 1930), professor at University of Alaska Fairbanks. He was the director of the International Arctic Research Center from 1998 to 2007, and is known for studies of the aurora borealis.[2] The official naming citation was published by the Minor Planet Center on 30 March 2010 (M.P.C. 69491).[9]

Notes

  1. ↑ 1.0 1.1 Pravec (2007): lightcuve plot for (4949) Akasofu, with a rotation period 2.6800±0.0003 hours with a brightness amplitude of 0.15 magnitude. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 4949 Akasofu (1988 WE)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004949. 
  2. ↑ 2.0 2.1 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (4949) Akasofu. Springer Berlin Heidelberg. p. 402. ISBN 978-3-540-29925-7. https://books.google.com/books?id=aeAg1X7afOoC&pg=PA402. Retrieved 30 December 2015. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (4949) Akasofu". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=4949%7CAkasofu. 
  4. ↑ 4.0 4.1 4.2 4.3 Mainzer, 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M. Retrieved 3 May 2016. 
  5. ↑ 5.0 5.1 5.2 Masiero, 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. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 5 December 2016. 
  6. ↑ 6.0 6.1 Higgins, 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. ISSN 1052-8091. Bibcode: 2006MPBu...33....8H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006MPBu...33....8H. Retrieved 3 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 3 May 2016. 
  8. ↑ 8.0 8.1 "4949 Akasofu (1988 WE)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=4949. 
  9. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 

External links



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