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G-type asteroid
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{{Multiple issues| {{refimprove|date=June 2014}} {{One source|date=February 2024}} {{No footnotes|date=February 2024}} }} [[File:PIA19562-Ceres-DwarfPlanet-Dawn-RC3-image19-20150506.jpg|thumb|right|[[Ceres (dwarf planet)|Ceres]], the largest asteroid, is a G-type]] '''G-type asteroids''' are a relatively uncommon type of [[carbon]]aceous [[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 asteroid#Characteristics|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 mineral]]s such as [[clay]]s or [[mica]]. In the [[asteroid spectral types#SMASS classification|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 asteroid|C-type]] and some rare types are sometimes collected together into a wider [[C-type asteroid#C-group asteroids|C-group]] of [[carbon]]aceous asteroids. ==See also== * [[Asteroid spectral types]] ==References== * D. J. Tholen Asteroid taxonomic classifications in Asteroids III {{Reflist}} {{Asteroids}} {{Small Solar System bodies}} {{DEFAULTSORT:G-Type Asteroid}} [[Category:Asteroid spectral classes]] [[Category:G-type asteroids (Tholen)|*]] {{asteroid-stub}}
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