G-type asteroid

From Wikipedia, the free encyclopedia
Revision as of 16:59, 4 February 2024 by imported>Emir of Wikipedia (Added {{One source}} and {{No footnotes}} tags)
(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search

Template:Multiple issues

File:PIA19562-Ceres-DwarfPlanet-Dawn-RC3-image19-20150506.jpg
Ceres, the largest asteroid, is a G-type

G-type asteroids are a relatively uncommon type of carbonaceous asteroid that makes up approximately 5% of asteroids. The most notable asteroid in this class is 1 Ceres.

Characteristics

Generally similar to the C-type objects, but contain a strong ultraviolet absorption feature below 0.5 μm. An absorption feature around 0.7 μm may also be present, which is indicative of phyllosilicate minerals such as clays or mica.

In the SMASS classification the G-type corresponds to the Cgh and Cg types, depending on the presence or absence (respectively) of the absorption feature at 0.7 μm. The G-type, C-type and some rare types are sometimes collected together into a wider C-group of carbonaceous asteroids.

See also

References

  • D. J. Tholen Asteroid taxonomic classifications in Asteroids III

Template:Reflist

Template:Asteroids Script error: No such module "Navbox".

Template:Asbox