Panel (a): H–R diagram of the open cluster members stars with GALEX observations. The blue solid line is the fitting results of main sequences. green dashed lines represent the upper
Panel (a): H–R diagram of the open cluster members stars with GALEX observations. The blue solid line is the fitting results of main sequences. green dashed lines represent the upper
The (Origin of) Life Marker Chip (LMCOOL) — University of Twente Is life possible – or has it ever been possible – on other planets? The (Origin of) Life Marker
Continuum-subtracted ALMA observations of Titan on 2022-09-06, showing the spectrally integrated line flux maps for the CH3CN J = 35 − 34 and J = 36 − 35 bands (left
Observed spectra after dividing by the out-of-transit spectrum (residuals), shown in the stellar rest frame. Vertical orange and green dotted lines indicate the positions of the Na D2 and D1
The result of applying the trained Planet-FP SOMs on their respective training data. The plots showcase the position of each training event on the SOM pixel map with some added
Simulation results from HD 134987 exploratory runs with synthetic data created at future epochs using four variables and real data from Jones et al. (2010). The Pmax uncertainty before the
Slices from the edge of Mars reveal a layered atmosphere of delicate complexity. A European spacecraft has captured a luminous mille-feuille of dust enveloping the Red Planet in unprecedented detail.
Image: Graphic of the heliosphere, a bubble in space created as the solar wind flows away from the sun. (Credit: NASA/IBEX/Adler Planetarium) A scientific instrument from Colorado is scheduled to
This chart shows, on the top row, artist concepts of the seven planets of TRAPPIST-1 with their orbital periods, distances from their star, radii, masses, densities and surface gravity as
Formic acid, HCOOH — Wikipedia Context. Nonthermal desorption from interstellar ices induced by X-rays, known as X-ray photodesorption, is a possible route to explain gas phase molecules detected in protoplanetary