Results 111 to 120 of about 24,858 (303)
NASA Laboratory Astrophysics Workshop 2006 Introductory Remarks
, 2006 NASA Laboratory Astrophysics Workshop 2006, is the fourth in a series of workshops held at four year intervals, to assess the laboratory needs of NASA's astrophysics missions - past, current and future. Investigators who need laboratory data to interpret
Hasan, Hashima
core
Meteoritics &Planetary Science, EarlyView.Abstract Since the discovery of nine meteorites near the Yamato mountains in 1969, Antarctica has been recognized as a superb location for meteorite recovery. While Antarctic recovery expeditions prioritize meteorite preservation for mineralogical and planetary studies, meteorites are not typically collected for biological applications.
Rachael Lappan +2 more
wiley +1 more source
The Astrophysical JournalThe molecule, 2-cyanoindene, C _10 H _7 N (2CNI) is the only cyanosubstituted polycyclic aromatic hydrocarbon (PAH) detected in space, for which the hydrocarbon counterpart, indene, has also been observed in the same astrochemical environment—the ...
Arun Subramani +14 more
doaj +1 more source
NASA's Laboratory Astrophysics Workshop: Opening Remarks
, 2002 The Astronomy and Physics Division at NASA Headquarters has an active and vibrant program in Laboratory Astrophysics. The objective of the program is to provide the spectroscopic data required by observers to analyze data from NASA space astronomy ...
Hasan, Hashima
core
Meteoritics &Planetary Science, EarlyView.Abstract Near‐Earth rubble‐pile asteroids Bennu and Ryugu are part of the carbonaceous taxonomic complex (C‐complex), and samples returned from both bodies resemble the most aqueously altered carbonaceous chondrites. However, telescopic and spacecraft visible–near infrared (VIS–NIR) reflectance spectra of Ryugu exhibit a red (positive) spectral slope ...
Ralph E. Milliken +10 more
wiley +1 more source
Business Meeting Commission B5 Laboratory Astrophysics - IAU GA 2018
, 2018 Business Meeting Commission B5 Laboratory Astrophysics - IAU GA 2018 Presentation by ...
Salama, Farid
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Stardust Mine: A 2024 gabbroic shergottite from Arizona, USA
Meteoritics &Planetary Science, EarlyView.Abstract This study provides an initial characterization of Stardust Mine, a fresh gabbroic enriched shergottite collected in Arizona, USA, in September 2024 and is the first Martian meteorite to be unequivocably collected on US soil. Analysis was conducted on the type specimen and finds that Stardust Mine is composed of equal proportions of pyroxene ...
Jennifer T. Mitchell +4 more
wiley +1 more source
The A2Π–X2Σ+ Band System of ScO for M-type Star Spectral Analysis
The Astrophysical JournalM-type stars are the most abundant stars in our Galaxy. Their visible spectra are characterized by strong TiO and VO absorption bands with occasional ScO bands near 6000–6100 Å.
Léo Lavy +2 more
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Nuclear astrophysics in underground laboratories: The LUNA experiment [PDF]
AIP Conference Proceedings, 2019 Abstract One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions responsible for powering the stellar engine and for the synthesis of the chemical elements. At astrophysical energies the cross section of nuclear processes is extremely reduced by the effect of the Coulomb barrier.
openaire +2 more sources
ASTROLAB: A First Year Laboratory in Astronomy and Astrophysics
, 2003 ASTROLAB is a laboratory course for first year students on a physics and astrophysics degree programme at the University of Birmingham, UK. The laboratory runs for nine weeks with 5 h sessions.
Elliot, Ken H., Elliott, Kenneth
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