Astronomy:3988 Huma

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3988 Huma
Discovery [1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date4 June 1986
Designations
(3988) Huma
Pronunciation/ˈhmə/[3]
Named afterHuma bird
(Persian mythology)[2]
1986 LA
Minor planet categoryAmor · NEO[1][2]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc29.61 yr (10,815 days)
|{{{apsis}}}|helion}}2.0335 AU
|{{{apsis}}}|helion}}1.0556 AU
1.5445 AU
Eccentricity0.3166
Orbital period1.92 yr (701 days)
Mean anomaly61.265°
Mean motion0° 30m 48.6s / day
Inclination10.768°
Longitude of ascending node229.82°
86.912°
Earth MOID0.1781 AU · 69.4 LD
Physical characteristics
Dimensions0.7 km[1]
0.782 km (calculated)[4]
Rotation period10.4±0.1 h[lower-alpha 1]
Geometric albedo0.20 (assumed)[4]
S[4]
Absolute magnitude (H)17.9[1][4] · 17.97±0.15[5] · 18.17±0.29[6]


3988 Huma, provisional designation 1986 LA, is an eccentric sub-kilometer asteroid and near-Earth object of the Amor group. It was discovered on 4 June 1986, by American astronomer Eleanor Helin at Palomar Observatory, California.[2] The asteroid measures approximately 700 to 800 meters in diameter and was named after the Huma bird from Iranian mythology.

Orbit and classification

Huma is a stony S-type asteroid that orbits the Sun in the inner main-belt at a distance of 1.1–2.0 AU once every 1 years and 11 months (701 days). Its orbit has an eccentricity of 0.32 and an inclination of 11° with respect to the ecliptic.[1] As no precoveries were taken, the body's observation arc begins with its discovery observation at Palomar in 1986.[2]

It has an Earth minimum orbit intersection distance of 0.1781 AU (26,600,000 km), which corresponds to 69.4 lunar distances.[1]

Physical characteristics

Rotation period

A rotational lightcurve of Huma was obtained by American astronomer Brian A. Skiff in July 2011. It gave a rotation period of 10.4±0.1 hours with a brightness variation of 0.24 magnitude ({{{1}}}).[lower-alpha 1]

Diameter and albedo

In the 1990s, Dutch–American astronomer Tom Gehrels estimated Huma to measure 0.7 kilometers in diameter, based on an assumed medium albedo of 0.15. More recently, the Collaborative Asteroid Lightcurve Link assumed a standard albedo for stony asteroids of 0.20 and calculated a diameter of 0.78 kilometers.[4]

Naming

This minor planet was named after the Huma bird from Persian mythology and Sufi poetry. The mythological bird never alights on the ground, and its appearance in the sky is said to be a sign of fortune. The asteroid's name was suggested by the SGAC Name An Asteroid Campaign[2] and its citation was published on 9 September 2014 (M.P.C. 89832).[7]

Notes

  1. 1.0 1.1 Skiff (2011) web: rotation period 10.4±0.1 hours with a brightness amplitude of 0.24 mag. Skiff, B.A. (2011) Posting on CALL web site. Summary figures for (3988) Huma at Collaborative Asteroid Lightcurve Link (CALL)

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "JPL Small-Body Database Browser: 3988 Huma (1986 LA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003988. 
  2. 2.0 2.1 2.2 2.3 2.4 "3988 Huma (1986 LA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=3988. 
  3. huma (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=huma  (Subscription or UK public library membership required.)
  4. 4.0 4.1 4.2 4.3 4.4 "LCDB Data for (3988) Huma". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=3988%7CHuma. 
  5. Hicks, M.; Truong, T.; Gerhart, C.; McCormack, M.; Strojia, C.; Teague, S. (June 2011). "Broadband photometry of 3988 (1986 LA): A large low-V near-Earth Asteroid". The Astronomer's Telegram 3457 (3457): 1. Bibcode2011ATel.3457....1H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ATel.3457....1H. Retrieved 27 September 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. doi:10.1016/j.icarus.2015.08.007. Bibcode2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 27 September 2016. 
  7. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 

External links