Fullerene C60 — Wikipedia Fullerenes of extra-terrestrial origin may have been accessible as carbon sources for anaerobic microorganisms on the early Earth. Very little is known about how anaerobic microorganisms
Fullerene C60 — Wikipedia Fullerenes of extra-terrestrial origin may have been accessible as carbon sources for anaerobic microorganisms on the early Earth. Very little is known about how anaerobic microorganisms
ID: ESP_063775_1295, date: 4 March 2020, altitude: 251 km NASA/JPL-Caltech/University of Arizona Larger image Gullies are common on steep slopes of many impact craters on Mars. When gullies were first
Ann Nguyen, co-lead author of a new paper that gives insights into the diverse origin of asteroid Bennu’s “parent” asteroid works alongside the NanoSIMS 50L (nanoscale secondary ion mass spectrometry)
NASA Spaceline Current Awareness List — grok via Astrobiology.com SPACELINE Current Awareness Lists are distributed via listserv and are available on the NASA Task Book website at https://taskbook.nasaprs.com/tbp/spaceline.cfm. Please send any correspondence
Air sampling during a dust storm. Credit: Naama Lang-Yona How do living bacteria survive on the surface of dust particles carried by desert storms from the Sahara and Egypt to
A scanning electron microscope image of a micrometeorite impact crater in a particle of asteroid Bennu material. Credit NASA Asteroid Bennu — the target of NASA’s OSIRIS-REx sample return mission,
Snapshot of the triple transit of planet b, c, and d as seen by K2 at the end of 2016. This artistic representation has been created with the software tango
Results from the injection-recovery test for the helium envelope with a variable opacity. The top panel shows the inputted absorbance profiles (red curves), together with the empirically-retrieved absorbance profiles (red
Fractional abundances of PAHs as a function of the number of carbon atoms 𝑁C. Dotted lines denote the estimated abundance upper limits of large quasi-symmetric PAHs in NGC 7027, and
The Aurora Australis, photographed over Concordia station in July 2025, during the ongoing solar activity maximum, the peak of the Sun’s 11-year cycle. ESA – Larger image This dazzling light