dc.date.accessioned
2024-09-30T08:19:04Z
dc.date.available
2024-09-30T08:19:04Z
dc.identifier
https://doi.org/10.35003/2JF3BG
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/45072
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-44784
dc.description
Highlights:</br>
• Ryugu sample A0008 is spectrally most similar to CI chondrites.</br>
• C1/C2 clasts are distinguishable from CI chondrites due to differences in phyllosilicate composition.</br>
•The degree of aqueous alteration has a prominent effect on the MIR spectrum.
dc.subject
Asteroid Ryugu
dc.subject
carbonaceous chondrites
dc.subject
volatile-rich chondrites
dc.subject
infrared spectroscopy
dc.title
Replication Data for: Micro-FTIR reflectance spectroscopy of Ryugu, CI chondrites and volatile-rich clasts – Comparing spectral features in the Mid-IR (2.5–16.5 μm) region
dcterms.accessRights.openaire
metadata only access