Distribution of sample locations across sabkha units of different ages along the northern coast of the United Arab Emirates. (a) Sampling locations at various outcrops, including Sample A from modern
Distribution of sample locations across sabkha units of different ages along the northern coast of the United Arab Emirates. (a) Sampling locations at various outcrops, including Sample A from modern
The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Matheson BE, Walle M, Liphardt A-M, Hulme PA, Heer M,
Aram Chaos., Mars Credit: NASA/JPL-Caltech/University of Arizona. New research published in Nature Communications identifies an iron sulfate on Mars that may represent a brand-new mineral. Sulfur is common on Mars
(A) Sampling information and morphological characteristics of 11 deep-sea species. These samples were captured from depths ranging between 1,218 and 7,730 m, spanning locations from the Mariana Trench to the
Astrochemical reaction network.– Intelligent Computing Decoding cosmic evolution depends on accurately predicting the complex chemical reactions in the harsh environment of space. Traditional methods for such predictions rely heavily on
This view of tracks trailing NASA’s Curiosity was captured July 26, 2025, as the rover simultaneously relayed data to a Mars orbiter. Combining tasks like this more efficiently uses energy
Spread of niche constructors across a metapopulation through diffusion This simulation introduces the diffusion of units across microenvironments. During each extinction event, individual molecules have 1% chance of being sent
Molecular complexity growth rate per bond count between PubChem and COCONUT 2.0 molecules. Mean (solid line) and standard deviation (shaded area) of complexity scores per bond count between PubChem molecules
25.3 µm map of the NGC 7538 region from SOFIA/Faint Object infraRed Camera (FORCAST; Herter et al. 2013) archival data (Cycle 1 Program 0034, PI A. G. G. M. Tielens).
Examples of training reflection spectra for Earth-like exoplanets in the Archean (left), Proterozoic (center), and Modern (right) eras, observed with LUVOIR-B (top row) and Habex/SS (bottom row). Colored lines represent