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JWST-MIRI MRS spectrum of the young J0438 disk (black). The spectrum is dominated by amorphous silicate absorption and emission bands typical of a highly inclined disk configuration. A very weak

Orbital distribution of 7,982 impacts detected by EDMOND, CAMS, GMN, FRIPON, and EFN networks. Each impact is estimated to be equal to or greater than 10 g (diameter ⪆2 cm)

GJ1061 system – exoplanets GJ1061 b, GJ1061 c, GJ1061 d — NASA/Wikipedia GJ1061 is a very nearby M star hosting three low-mass temperate planets detected from radial velocity variations. The

Images of Jyvaskylavirus. The virus particle is about twice the size of influenza or coronavirus. — eLife For the first time in Finland, researchers at the Nanoscience Center in University

This image from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) of star-forming region NGC 604 shows how stellar winds from bright, hot, young stars carve out cavities in surrounding

Correlative images of a eukaryotic cell expressing native fluorescence captured by DHM amplitude and VFI intensity. The images are captured over 4 s (60 frames) and volume reconstructed. The DHM

A meteorite entering Earth’s atmosphere — Grok via Astrobiology.com An international team of researchers may have answered one of space science’s long-running questions – and it could change our understanding

An SwRI-led study modeled the chemistry of TOI-270 d, a nearby exoplanet between Earth and Neptune in size, finding evidence that it is a giant rocky world (super-Earth) surrounded by

Computer simulation of a one-sided magnetic field on early Mars based on data from a study led by the University of Texas Institute for Geophysics. The study could explain the