In search of Bennu analogs: Hapke modeling of meteorite mixtures

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Volume 648 (April 2021)

A&A, 648 (2021) A88

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Table 1

Material used to generate new optical constants.

From absorbance data
CI chondrite
Ivuna CI1	Orgueil CI1

CR chondrite
GRA 06100 CR2	GRO 03116 CR2	GRO 95577 CR1	LAP 02342 CR2

CM chondrite
ALH 83100 CM1/2	ALH 84044 CM2	Boriskino CM2	DOM 08003 CM2	EET 96029 CM2
LEW 85311 CM2-an	LEW 87022 CM2	LON 94101 CM2	MCY 05230 CM2	MIL 07700 CM2
Murchison CM2	Niger CM2	Nogoya CM2	PCA 91008 CM2-an	QUE 99355 CM2
QUE 97990 CM2	WIS 91600 CM-an

CV chondrite
Grosnaja CV3	Kaba CV3	Mokoia CV3	Vigarano CV3

C2-ungrouped chondrite
Bells	Essebi

CK chondrite
ALH 85002 CK4	Maralinga CK4-an	EET 92002 CK5

From reflectance data
Alais CI1	Crescent CM2	EET 83226 C2-ung	Essebi C2-ung	Mokoia CV3
Murchison CM2	Orgueil CI1	Tagish Lake C2-ung

Notes. ALH = Allan Hills, DOM = Dominion Range, EET = Elephant Moraine, GRA = Graves Nunatak, GRO = Grosvenor Range, LAP = LaPaz, LEW = Lewis Cliff, LON = Lonewolf Nunataks, MCY = MacKay Glacier, MET = Meteorite Hills, MIL = Miller Range, PCA= Pecora Escarpment, and WIS = Wisconsin Range.

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