Optical Hubble Space Telescope (HST) images of the targets NGC 4321 (top) and M51 (bottom) overlaid with CO, HCN and SFR contours (from left to right). The CO (HCN) contours
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From Gas To Stars Along The Spiral Wave: CO, HCN, And Star Formation Variations Across The Spiral Arms In NGC 4321 And M51
Optical Hubble Space Telescope (HST) images of the targets NGC 4321 (top) and M51 (bottom) overlaid with CO, HCN and SFR contours (from left to right). The CO (HCN) contours
Finding Alien Worlds in Queensland — A Decade of MINERVA-Australis
This image shows the MINERVA-Australis array located at the Mount Kent Observatory in Australia. — NASA Three decades ago, humanity entered the Exoplanet Era, with the discovery of the first
A Single Power Law For The TRAPPIST-1 Flare Distribution Across Four Orders Of Magnitude In Energy
Cumulative flare-frequency distribution of TRAPPIST-1. The cumulative occurrence rate ν(≥ ETESS) is shown as a function of TESS-band flare energy. The K2 FFD from this work is shown in blue,
Phase-Space Crystallization in Galactic Globular Clusters: A Gaia-Based Metric and Implications for Technosignature Searches
Correlations of crystallization metrics with cluster mass, Galactocentric distance, and a dynamical-age proxy. Top row: Cindex versus log(Mcl/M⊙), RGC, and log10(tage/trh). Bottom row: the N⋆-corrected residual index Cresid versus the
A Preliminary Exploration Of The Effects Of Baseline Length For The LIFE Space Mission
Integration time required for an Earth-twin around a given star to reach an SNR of 7, plotted as a function of stellar parameters. The baseline limits are set at 25-80
Night Sky: A Field Guide to the Constellations
In the vast expanse of our universe, where stars whisper secrets of the cosmos, “Night Sky: A Field Guide to the Constellations” emerges as an essential companion for those yearning
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This image shows the MINERVA-Australis array located at the Mount Kent Observatory in Australia. — NASA Three decades ago, humanity entered the Exoplanet Era, with the discovery of the first
Cumulative flare-frequency distribution of TRAPPIST-1. The cumulative occurrence rate ν(≥ ETESS) is shown as a function of TESS-band flare energy. The K2 FFD from this work is shown in blue,
Correlations of crystallization metrics with cluster mass, Galactocentric distance, and a dynamical-age proxy. Top row: Cindex versus log(Mcl/M⊙), RGC, and log10(tage/trh). Bottom row: the N⋆-corrected residual index Cresid versus the
Integration time required for an Earth-twin around a given star to reach an SNR of 7, plotted as a function of stellar parameters. The baseline limits are set at 25-80
In the vast expanse of our universe, where stars whisper secrets of the cosmos, “Night Sky: A Field Guide to the Constellations” emerges as an essential companion for those yearning
WASHINGTON — The Space Systems Command’s commercial space office awarded Viasat a $307 million contract to provide satellite communications services for the U.S. Marine Corps. The company is retaining the
Spring is here and with it, a new set of sparkling constellations rises to prominence! But what are the stories behind these mesmerizing stellar citadels and how can you find
Astronauts for America – The Best of the Best Speak Out – YouTube Watch On On Episode 209 of This Week In Space, Rod Pyle and Tariq Malik talk with
The pioneering Voyager probes might only have a few years left to explore interstellar space, and that’s assuming a planned, risky maneuver in 2026 goes well. NASA’s twin Voyager 1
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