Astronomy:12621 Alsufi

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12621 Alsufi
Discovery[1]
Discovered byC. J. van Houten
I. van Houten-G.
Tom Gehrels
Discovery sitePalomar Obs.
Discovery date24 September 1960
Designations
(12621) Alsufi
Named afterAbd al-Rahman al-Sufi
(astronomer)[2]
6585 P-L · 1997 JJ12
Minor planet categorymain-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc56.33 yr (20,576 days)
|{{{apsis}}}|helion}}3.5148 AU
|{{{apsis}}}|helion}}2.6980 AU
3.1064 AU
Eccentricity0.1315
Orbital period5.48 yr (2,000 days)
Mean anomaly142.13°
Mean motion0° 10m 48s / day
Inclination2.4308°
Longitude of ascending node148.06°
204.34°
Physical characteristics
Dimensions6.76 km (calculated)[3]
Rotation period4.7194±0.0024 h[4]
Geometric albedo0.08 (assumed)[3]
L[5] · C[3]
Absolute magnitude (H)13.9[1] · 13.91±0.26[5] · 13.761±0.014 (R)[4] · 14.21[3]


12621 Alsufi, provisionally designated 6585 P-L, is a carbonaceous Themistian asteroid from the outer region of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by astronomers during the Palomar–Leiden survey in 1960, and named for medieval Persian astronomer Abd al-Rahman al-Sufi.

Discovery

Alsufi was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at the U.S. Palomar Observatory, California.[6] No precoveries were taken prior to its discovery observation.[6]

Palomar–Leiden survey

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[7]

Classification and orbit

It is a member of the Themis family, a dynamical group of outer-belt asteroids with nearly coplanar ecliptical orbits. The C-type asteroid is also classified as a rather rare L-type asteroid by Pan-STARRS' large-scale survey.[5] It orbits the Sun in the outer main-belt at a distance of 2.7–3.5 AU once every 5 years and 6 months (2,000 days). Its orbit has an eccentricity of 0.13 and an inclination of 2° with respect to the ecliptic.[1]

Physical characteristics

A rotational lightcurve of this asteroid was obtained from photometric observations made at the U.S. Palomar Transient Factory, California, in January 2012. It gave a rotation period of 4.7194±0.0024 hours with a brightness amplitude of 0.71 in magnitude ({{{1}}}).[4] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 6.8 kilometers with an absolute magnitude of 14.21.[3]

Naming

This minor planet is named in honor of 10th-century Persian astronomer Abd al-Rahman al-Sufi (A.D. 903–986), also known by his western name, Azophi. Working in Isfahan, he produced his influential star atlas around A.D. 963. The atlas is based on both, Ptolemy's Almagest and on pre-Islamic star lore, and contains the earliest description of the Andromeda Galaxy.[2] The approved naming citation was published by the Minor Planet Center on 22 January 2008 (M.P.C. 61764).[8] The lunar crater Azophi is also named in his honour.

References

  1. 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 12621 Alsufi (6585 P-L)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2012621. Retrieved 5 July 2017. 
  2. 2.0 2.1 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (12621) Alsufi. Springer Berlin Heidelberg. p. 823. ISBN 978-3-540-29925-7. https://books.google.com/books?id=aeAg1X7afOoC&pg=PA823. Retrieved 13 May 2016. 
  3. 3.0 3.1 3.2 3.3 3.4 3.5 "LCDB Data for (12621) Alsufi". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=12621%7CAlsufi. Retrieved 13 May 2016. 
  4. 4.0 4.1 4.2 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal 150 (3): 35. doi:10.1088/0004-6256/150/3/75. Bibcode2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 13 May 2016. 
  5. 5.0 5.1 5.2 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 13 May 2016. 
  6. 6.0 6.1 "12621 Alsufi (6585 P-L)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=12621. Retrieved 13 May 2016. 
  7. "Minor Planet Discoverers". Minor Planet Center. 28 December 2015. https://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html. Retrieved 13 May 2016. 
  8. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 13 May 2016. 

External links