Astronomy:47 Aglaja

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Short description: Main-belt asteroid
47 Aglaja
Aglaja (asteroid).jpg
An image of Aglaja taken by the SDSS telescope on 13 October 1999. The minor planet was 1.7 AU from Earth at the time of photography.
Discovery
Discovered byRobert Luther
Discovery dateSeptember 15, 1857
Designations
(47) Aglaja
Pronunciation/əˈɡl.ə/[2]
Named afterAglaea
Aglaia[1]
Minor planet categoryMain belt
AdjectivesAglajan
Orbital characteristics[3]
Epoch December 31, 2006 (JD 2454100.5)
|{{{apsis}}}|helion}}488.740 Gm (3.267 AU)
|{{{apsis}}}|helion}}372.222 Gm (2.488 AU)
430.481 Gm (2.878 AU)
Eccentricity0.135
Orbital period1,782.960 d (4.88 a)
Mean anomaly225.007°
Inclination4.985°
Longitude of ascending node3.244°
314.589°
Physical characteristics
Dimensions141.90 ± 8.72 km[4]
Mass(3.25±1.68)×1018 kg[4]
Mean density2.17 ± 1.19 g/cm3[4]
Rotation period13.175[5] h
Geometric albedo0.080 [6]
C (Tholen)
B (SMASSII)[7]
Absolute magnitude (H)7.84


47 Aglaja /əˈɡl.ə/ is a large, dark main belt asteroid. It was discovered by Robert Luther on 15 September 1857 from Düsseldorf.[8] The name was chosen by the Philosophical Faculty of the University of Bonn and refers to Aglaea, one of the Charites in Greek mythology.[9] It was rendered Aglaia in English sources into the early 20th century, as 'i' and 'j' are equivalent in Latin names and in the Latin rendering of Greek names.[1]

Based upon its spectrum, 47 Aglaja is listed as a C-type asteroid under the Tholen classification taxonomy, indicating a carbonaceous composition. The SMASS classification system rates it as a rare B-type asteroid. There is a broad absorption feature at 1 μm that is associated with the presence of magnetite and is what gives the asteroid its blue tint.[7]

On 16 September 1984, the star SAO 146599 was occulted by 47 Aglaja. This event was observed from 13 sites in the continental United States, allowing a cross-sectional profile to be determined. Based upon this study, the asteroid has a diameter of 136.4 ± 1.2 km. The geometric albedo calculated at the time of the occultation was 0.071 ± 0.002.[10]

2012 photometric observations of this asteroid at the Organ Mesa Observatory in Las Cruces, New Mexico gave a light curve with a period of 13.175 ± 0.002 hours and a brightness variation of 0.09 ± 0.01 in magnitude. This result is in agreement with previous studies.[5]

References

  1. 1.0 1.1 John Craig (1869) The Universal English Dictionary
    Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  2. 'Aglaia' in Noah Webster (1884) A Practical Dictionary of the English Language
  3. Yeomans, Donald K., "47 Aglaja", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=47, retrieved 2013-04-07. 
  4. 4.0 4.1 4.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  5. 5.0 5.1 Pilcher, Frederick (October 2012), "Rotation Period Determinations for 47 Aglaja, 252 Clementina, 611 Valeria, 627 Charis, and 756 Lilliana", Minor Planet Bulletin 39: pp. 220–222, Bibcode2012MPBu...39..220P. 
  6. "Asteroid Data Sets". http://www.psi.edu/pds/resource/albedo.html. 
  7. 7.0 7.1 Yang, Bin; Jewitt, David (September 2010), "Identification of Magnetite in B-type Asteroids", The Astronomical Journal 140 (3): pp. 692–698, doi:10.1088/0004-6256/140/3/692, Bibcode2010AJ....140..692Y. 
  8. "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html, retrieved 2013-04-07. 
  9. Schmadel, Lutz (2003), Dictionary of minor planet names (fifth ed.), Germany: Springer, p. 19, ISBN 3-540-00238-3, https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA19, retrieved 2008-12-29. 
  10. Millis, R. L. et al. (October 1989), "The diameter, shape, albedo, and rotation of 47 Aglaja", Icarus 81: pp. 375–385, doi:10.1016/0019-1035(89)90058-4, Bibcode1989Icar...81..375M.  See Table 1.

External links