Disk physical structure from our three parametric models (Models 1 to 3 from top to bottom, see Tables 1 and 2). The 2D gas temperature (left) and total H density
Disk physical structure from our three parametric models (Models 1 to 3 from top to bottom, see Tables 1 and 2). The 2D gas temperature (left) and total H density
Variation of the planetary radius, expressed as transit depth, as a function of wavelength. Sky-blue points correspond to DanishDFOSC (this work), lime to TESS (this work), orange to GROND (Mancini
(A) The model of EnINpro is colored by different domains with arrows representing β strands. The model highlights a β-solenoid fold (gray, purple) adjacent to the disulfide capping motif (orange).
A Scanning Electron Microscope (SEM) micrograph of a SiGe transistor for use on ocean worlds. This SiGe IC is built from large numbers of micron-sized (10^-6 m) SiGe transistors to
Mg/Si ratios of JWST-observed hot Jupiter host stars versus separation (semi-major axis). Mg/Si ratios compiled from Brewer et al. (2016) with an error of 3.3% as quoted in Brewer &
Discover the Universe with Style: Ezcosplay Women’s Button Down Space Shirt Glimpse a world where fashion meets the cosmos with the Ezcosplay Women’s Button Down Space Shirt. This whimsical tee
NASA/Scott Eckley These X-ray computed tomography (XCT) scans released on March 17, 2026, give us a glimpse inside asteroid Bennu. They show the most common types of crack networks observed
Oxygen has been the most important gas in our search for life among the cosmos thus far. On Earth, we have it in abundance because it is produced by biological
5 Min Read Asteroid Bennu’s Rugged Surface Baffled NASA, We Finally Know Why These are X-ray computed tomography (XCT) scans of particles from asteroid Bennu. They show the most common
The bigger the hailstone, the more damage it can cause. But scientists find that predicting hailstone size can be challenging. How quickly does hail melt as it falls? Now, you






