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2018-07-17. Image taken with the Asiago Schmidt telescope with B, g, r filters. Comet Giacobini-Zinner moves fast in a very starrich field in the constellation Cygnus. The dust tail,
Binary collision-induced H2–He absorption coefficient, α, normalized by the hydrogen and helium gas densities, as function of frequency in the fundamental band, at 296 K. The parato-ortho distribution, is representative
Astronomers have used the James Webb Space Telescope (JWST) to study the dusty shrouds that envelope dying stars. The investigation could help reveal where vast amounts of cosmic dust come
An artist’s rendering of the warm exoplanet WASP-80 b and an overview of its planet-system parameters. Planet image credit: NASA/Ames Research Center. astro-ph.EP WASP-80 b, a warm sub-Jovian (equilibrium temperature
Displaying the sudden change in spectral features for oxygen-rich atmospheric spectra. Type B atmospheres spectra do not show any CH4 features, as do type C which are extremely oxygen-rich. Both
Artist’s concept of exoplanet HIP 67522 b, a planet with a death wish. It triggers flares of radiation from its star. Image via Danielle Futselaar/ ESA. Used with permission. Astronomers
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What imaging systems can NASA’s Artemis astronauts use on the Moon to conduct groundbreaking science and efficient documentation on the lunar surface? This is what a recent study presented at
There’s nothing more comforting for fans of a cherished sci-fi TV series than knowing another season (plus a fifth and final season) is being filmed even before the latest one
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