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,
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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
Phosphorus abundances as a function of fundamental stellar parameters for all sample stars. Upper panel: Phosphorus abundance as a function of Teff. Lower panel: Phosphorus abundance as a function of
Overview of the CHEOPS operational chain. The ground segment components, MOC and SOC, are represented by coloured boxes. The orange arrows describe the weekly operations from reviewing and ingesting the
Transformations between the ORF (blue), SRF (orange), and BRF (green), with Euler angles. The SRF and the BRF are both rotating frames, with ZS the spin axis of Venus and
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