Thiocarbonic acid — astro-ph.GA The first experimental formation of thiocarbonic acid (H2CS3) is presented in this work from low-temperature interstellar ice analogs composed of hydrogen sulfide (H2S) and carbon disulfide

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.