Overview of the chemical elements detected in the transmission spectra of Ultra-Hot Jupiters (UHJ). Planets are ordered by decreasing equilibrium temperature. WASP-33 b is a more challenging target due to
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NASA/JPL-Caltech NASA’s Perseverance rover captured this view of Deimos, the smaller of Mars’ two moons, shining in the sky at 4:27 a.m. local time on March 1, 2025, the 1,433rd
Texas is positioning itself at the forefront of human spaceflight research with a $1 billion proposal to upgrade NASA’s Johnson Space Center, preparing the facility to support long-duration missions to
Join us on June 10 for an exclusive one-on-one conversation with Representative George Whitesides (D-CA), a freshman congressman representing California’s 27th District. Whitesides brings years of experience to Capitol Hill,
Call it an SOSS message – a Save Our Solar System planetary science community communiqué. It is unquestionably a “wait-a-minute” concern running through the space science research groups. Given the
In this week’s episode of Space Minds Mamta Patel Nagaraja – NASA’s former associate chief scientist-offers an insider’s look at how science priorities are set, what gets cut
6 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) Sunlight reflects off the ocean surface near Norfolk, Virginia, in this 1991 space shuttle image, highlighting swirling patterns created
2 min read Space Cloud Watch Needs Your Photos of Night-Shining Clouds Noctilucent Clouds observed from Bozeman, MT on 16 July 2009 at 4:29 MDT. The Space Cloud Watch project
The HPF-SpecMatch spectra fit results for order index 5. Top: two plots showing the five best-fit stars (red) selected to compose the spectra. The size and transparency of these five
Displaying the sudden change in spectral features for oxygen-rich atmospheric spectra. Type B atmospheres spectra do not show any CH4 features, as do type C which are extremely oxygen-rich. Both
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