Astrobiology35- Page

JWST GO time allocation for exoplanet science on different Cycles. Representation of the total General Observer (GO) allocated time for exoplanet science on JWST Cycle 1 (released on March, 2021,

HZ prescriptions used in this work: runaway greenhouse IHZ and maximum greenhouse OHZ from Kopparapu et al. (2014); water condensation limit IHZ from Turbet et al. (2023). Over-plotted are the

The Rossiter-McLaughlin effect of WASP-129 Ab, WASP-162b, Qatar-7b, and EPIC 219388192b. The observed data points (black) are shown with their error bars. The systemic and Keplerian orbit velocities were removed.

The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Hill MS, Minnis VR, Simpson AC, Salas Garcia MC, Bone

The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Lim S, Veres JE, Almeida EAC, O’Connell GD.Characterization of the

NASA 2025 Virtual Space Biosciences Training Call for Applications Number: NNH25ZDA011LResponse Due Date: July 9, 2025 Short URL: https://go.nasa.gov/ApplySTAR25 NASA invites applications for the 6th cohort of the Spaceflight Technology,

Gas-phase C/O ratio as a function of distance to the star for the two different values of the stellar mass (M∗ = 1, 0.1 M⊙) and three values of the

Evolution of the number of planets in one system averaged over 20 runs, ⟨Np⟩. The horizontal axes are the time normalized by the Kepler period of the innermost planet in

Illustration of the various probabilities discussed. The variable x may refer to any of the physical constants α, β, γ etc., with the others integrated over. The dashed lines indicate

Lander prototype during field tests at Matanuska Glacier, Alaska (Credit: NASA/JPL-Caltech) Europa, a moon of Jupiter, is a high-priority target for space exploration because of its potential to harbor life.