C/O ratio as a function of metallicity as given in Table 4. Planets observed with direct spectroscopy are shown as blue circles, planets observed with eclipse spectroscopy as magenta
C/O ratio as a function of metallicity as given in Table 4. Planets observed with direct spectroscopy are shown as blue circles, planets observed with eclipse spectroscopy as magenta
The normalized JWST spectra of the atomic PDR region and DF3 regions of the Orion Bar (black and red solid lines, respectively) after subtraction of the continuum and plateau emission.
Left: imaginary parts of tidal Love numbers, scaled by (Ω/ωdyn) 2ωt/Ω and plotted as a function of tidal frequency for isentropic polytropes (top) and incompressible shells (bottom) with a constant
Setup of our numerical simulations. Panel (A) illustrates an idealized icy moon with a poleward-thinning ice shell. Panel (B) depicts the numerical setup. — astro-ph.EP A poleward-thinning ice shell can
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Earth just endured one of its most extreme wildfire years on record — and scientists say human-driven climate change is the cause. A sweeping new analysis, the State of Wildfires
Key specs Camera: 1/1.3in CMOS & 16mm lens Video resolution: Up to 8K Frame rates: 8K up to 30 FPS, 4K up to 120 FPS, 10-bit HLG up to 60
In this episode of Space Minds, host David Ariosto speaks with Max Haot, CEO of Vast, the ambitious aerospace company based in Long Beach, California, one of a




