Impact history should play a crucial role in the search for habitable exoplanets like Earth — SwRI An SwRI-led team compared the early impact history of Venus and Earth, determining
Impact history should play a crucial role in the search for habitable exoplanets like Earth — SwRI An SwRI-led team compared the early impact history of Venus and Earth, determining
A clay-rich mesa in the Hellas basin of Mars. The blue color near the rim is aluminum bearing clays. The red-orange color below that is iron and magnesium bearing clays.
Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on
The Antarctic midge is the only known insect native to Antarctica. Credit Yuta Shimizu / Osaka Metropolitan University Picture an Antarctic animal and most people think of penguins, but there
Candidate targets for the Rocky Worlds DDT programme in the context of the ‘Cosmic Shoreline’, including the two first selected targets (highlighted in orange). Credit: Néstor Espinoza & Mees Fix
Galactic-scale properties of the sample. We plot against sin(|b|) EB−V (top left), N(HI) (top right), N(H2) = N(HCO+ )/3 × 10−9 (bottom left), and WCO, the line profile integral of
Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on
Analysis & Data Overview. (a) Top Left: Systematic-corrected signal image, for which a model fit is retrieved, which is shown in the central panel. Top Right: Spatially-flattened spectral profile of
The HHZ (blue shaded regions) and dark HHZ (red shaded regions) around a 0.12M⊙ star for a 7M⊕, 1.7R⊕ hycean planet with tidal quality factor Q = 2. The low-opacity
Spectra showing local sources of RFI that consistently affect the Parkes UWL bandpass. The UWL receiver records two polarisations which are represented by the colours red and blue, respectively, in