The aqueous alteration history in the solar system are studied through acquiring additional CCD reflectance spectra in the blue-UV through near-IR spectral region and analyzing these spectra for information about iron oxides in phyllosilicates identified in the CM and CI carbonaceous chondrites. Emphasis is on the main-belt and Cybele primitive asteroids, as these asteroids show spectral diversity and are also spectral analogues for known meteorite samples. The porphyrin bands found in organics near 0.4 micron is also sought
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...
The analysis of visible and near-infrared reflectance spectra is the primary means to determine surf...
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...
The composition of primitive asteroids and their relationship to satellites in the solar system will...
We investigated the petrologic, geochemical, and spectral parameters that relate to the type and deg...
The compositional distribution of asteroids provides clues to understanding solar system formation a...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
The highly hydrated, petrologic type 1 CM and CI carbonaceous chondrites likely derived from primiti...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
Small bodies in the Solar System preserve evidence of the processes occurring during early Solar Sys...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bo...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
The highly hydrated, petrologic type 1 CM and CI carbonaceous chondrites likely derived from primiti...
In the last year we have started a spectroscopic investigation of asteroids located in the region o...
Thesis (Ph. D.)--University of Hawaii at Manoa, 1983.Microfiche.xv, 201 leaves, bound ill. 29 cmThe ...
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...
The analysis of visible and near-infrared reflectance spectra is the primary means to determine surf...
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...
The composition of primitive asteroids and their relationship to satellites in the solar system will...
We investigated the petrologic, geochemical, and spectral parameters that relate to the type and deg...
The compositional distribution of asteroids provides clues to understanding solar system formation a...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
The highly hydrated, petrologic type 1 CM and CI carbonaceous chondrites likely derived from primiti...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
Small bodies in the Solar System preserve evidence of the processes occurring during early Solar Sys...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bo...
We analyse here a wide sample of carbonaceous chondrites from historic falls (e.g. Allende, Cold Bok...
The highly hydrated, petrologic type 1 CM and CI carbonaceous chondrites likely derived from primiti...
In the last year we have started a spectroscopic investigation of asteroids located in the region o...
Thesis (Ph. D.)--University of Hawaii at Manoa, 1983.Microfiche.xv, 201 leaves, bound ill. 29 cmThe ...
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...
The analysis of visible and near-infrared reflectance spectra is the primary means to determine surf...
Asteroids are relics from the early Solar System. Some of them are extremely primitive and can help ...