Line profiles of ionized emission from the outflow in the nuclear region of W2246- 0526, marked with a red circle in the inserted figure showing the extended Hα emission in
Line profiles of ionized emission from the outflow in the nuclear region of W2246- 0526, marked with a red circle in the inserted figure showing the extended Hα emission in
The temperature versus depth and time for 𝜅 = 10−4 W m−1 K−1 , 10−3 W m−1 K−1, and 10−2 W m−1 K−1 (top, middle, and bottom panels). The sublimation
NASA astronaut Chris Williams poses for an official portrait at the agency’s Johnson Space Center in Houston. Credit: NASA NASA will host a news conference at 2 p.m. EDT Wednesday,
Enceladus’ ice continues to get more and more intriguing as researchers continue to unlock more secrets taken from a probe over ten years ago. When Cassini crashed into Saturn in
The IMEWG (International Mars Exploration Working Group) is planning to stand up a sub-working group to identify international science and planetary protection goals and scope priorities in the upcoming transition
How do YOU say Astrobiology? — Grok via Astrobiology.com Editor’s note: I asked Grok to tell me how to say “astrobiology” in the top 100 languages spoken on Earth. The
Astronomers from the Aryabhatta Research Institute of Observational Sciences (ARIES) in India and elsewhere have conducted a long-term photometric and spectroscopic study of a young stellar object known as V1180
Threats from space aren’t always obvious, but statistically its only a matter of time before one of them happens. One of the most concerning for many space experts is a
The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Ferraro S, Sengupta S, Shaw J, Dave A, Cheli M,
Modifications to the Kepler survey completeness for our sample, based on the simulated presence of stellar companions using left: the properties of our observed companion sample at their observed rate






