Jump to content

423 Diotima

From Wikipedia

Template:Short description Template:Use dmy dates Template:Infobox planet

423 Diotima is one of the larger main-belt asteroids. It is classified as a C-type asteroid[1] and is probably composed of primitive carbonaceous material.

It was discovered by Auguste Charlois on 7 December 1896, in Nice. In the late 1990s, a network of astronomers worldwide gathered lightcurve data that was ultimately used to derive the spin states and shape models of 10 new asteroids, including 423 Diotima. The light curve for this asteroid varies "a lot" depending on the position, with the brightness variations ranging from almost zero to up to 0.2 in magnitude.[2][3] Dunham (2002) used 15 chords and obtained an estimated size of Template:Val.[4]

Name

Diotima is named for Diotima of Mantinea, a priestess who was one of Socrates's teachers. It is one of seven of Charlois's discoveries that was expressly named by the Astromomisches Rechen-Institut (Astronomical Calculation Institute).[5]

The name is stressed on the penultimate syllable, Template:IPAc-en Template:Respell, as in Latin Diotīma.

References

Template:Reflist

Template:Minor planets navigator Template:Small Solar System bodies Template:Authority control

  1. Cite error: Invalid <ref> tag; no text was provided for refs named jpldata
  2. Cite error: Invalid <ref> tag; no text was provided for refs named Durech2007
  3. Durech, J.; Kaasalainen, M.; Marciniak, A.; Allen, W. H. et al. "Asteroid brightness and geometry," Astronomy and Astrophysics, Volume 465, Issue 1, April I 2007, pp. 331-337.
  4. Template:Cite journal
  5. Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. Template:ISBN.