CARL — Credit John O. Dabiri and Peter Gunnarson An autonomous underwater vehicle can propel itself efficiently by using the energy in nearby water currents. Underwater and aerial vehicles must
CARL — Credit John O. Dabiri and Peter Gunnarson An autonomous underwater vehicle can propel itself efficiently by using the energy in nearby water currents. Underwater and aerial vehicles must
Artists concept of planet formation in the PDS 70 system.– The Graduate University for Advanced Studies/NAOJ A groundbreaking study by Canadian astronomers using the James Webb Space Telescope (JWST) has
The upper half of the figure illustrates the process of generating a molecular dication by doubly ionizing methanol via electron rescattering. The electric field of the ultrafast laser pulse (represented
(i, i-z) diagram of USco members (left) identified by MiretRoig et al. (2022) and Taurus members (right) from Esplin & Luhman (2019), represented as blue dots. The HST targets are
Distribution of the 11.0/11.2 PAH band ratio versus stellar effective temperature for our HAeBe sample. Reference stars (SR 21A, PDS 144N, HD 97300) shows different ionization regimes. The shaded regions
Reprocessed images of Uranus ] and Neptune NASA/JPL-Caltech (Uranus and Neptune); “Modelling the Seasonal Cycle of Uranus’s Colour and Magnitude, and Comparison with Neptune,” by Patrick G. J. Irwin
Exploration Crew Medical Officer – Grok via Astrobiology.com Introduction: Predictive analytics may be a useful adjunct to identify training needs for exploration class medical officers onboard deep space vehicles. Methods:
This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago.
Transit zones for all solar system planets are plotted in heliocentric ecliptic coordinates (left) and in celestial coordinates (right). Each planet’s transit zone is shown as a colored sinusoidal band.
SETI@home is a radio Search for Extraterrestrial Intelligence (SETI) project that looks for technosignatures in data recorded at the Arecibo Observatory. The data were collected over a period of 14