This article was originally published at The Conversation. The publication contributed the article to Space.com’s Expert Voices: Op-Ed & Insights. A new wave of climate research is sounding a stark
This article was originally published at The Conversation. The publication contributed the article to Space.com’s Expert Voices: Op-Ed & Insights. A new wave of climate research is sounding a stark
In a new study, scientists began pondering a pretty wild question: What if black holes can convert dead star matter into dark energy, the mystery force driving the acceleration of
A SpaceX Falcon 9 rocket lifts off from Space Launch Complex 40 at Cape Canaveral Space Force Station to begin SpaceX’s 33rd Commercial Resupply Services (CRS-33) mission to the International
NASA’s SpaceX 33rd commercial resupply mission successfully launched to deliver supplies and science investigations to the International Space Station from Space Launch Complex 40 at Cape Canaveral Space Force Station
A SpaceX Falcon 9 rocket stands at Space Launch Complex 40 at Cape Canaveral Space Force Station ahead of the launch of SpaceX’s 33rd Commercial Resupply Services (CRS-33) mission. Image:
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




