Английская Википедия:776 Berbericia

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Use dmy dates Шаблон:Infobox planet

776 Berbericia is a minor planet orbiting the Sun. A main-belt C-type asteroid,[1] it was discovered on 24 January 1914 by astronomer Adam Massinger at Heidelberg Observatory in southwest Germany. It was named by Max Wolf in honor of Adolf Berberich (1861–1920), a German astronomer.[2][3] The spectra of the asteroid displays evidence of aqueous alteration.[1]

Description

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 (776) Berbericia. The computed shape model for this asteroid is described as "asymmetric with sharp edges".[4][5]

Richard P. Binzel and Schelte Bus further added to the knowledge about this asteroid in a lightwave survey published in 2003. This project was known as Small Main-belt Asteroid Spectroscopic Survey, Phase II or SMASSII, which built on a previous survey of the main-belt asteroids. The visible-wavelength (0.435-0.925 micrometre) spectra data was gathered between August 1993 and March 1999.[6]

References

Шаблон:Reflist

External links

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


Шаблон:Beltasteroid-stub

  1. 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок Fornasier1999 не указан текст
  2. JPL Small-Body Database Browser
  3. Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. Шаблон:ISBN.
  4. Ошибка цитирования Неверный тег <ref>; для сносок Durech2007 не указан текст
  5. 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.
  6. Bus, S., Binzel, R. P. Small Main-belt Asteroid Spectroscopic Survey, Phase II. EAR-A-I0028-4-SBN0001/SMASSII-V1.0. NASA Planetary Data System, 2003.