Abundances (top) and correlation coefficients (bottom) of H2O, CO, CO2, CH3OH, and NH3 ices at T = 10 K, nH/ = 105 cm−3, ζ = 1.3 × 10−17s−1 and FUV
Abundances (top) and correlation coefficients (bottom) of H2O, CO, CO2, CH3OH, and NH3 ices at T = 10 K, nH/ = 105 cm−3, ζ = 1.3 × 10−17s−1 and FUV
Graphical Abstract. — ISME via PubMed Despite growing evidence for the role of DNA methylation in bacterial acclimation to environmental stress, this epigenetic mechanism remains unexplored in sea-ice microbial communities
Depiction of the reaction network of the C2H4 + CH2CCH+ reaction. The energies are calculated at the DLPNO-CCSD(T)/aug-cc-pvtz level with the ωB97XD/def2-TZVPD harmonic zero point energy. In the diagram EQ
Nicholas Ray, assistant professor in the School of Marine Science and Policy at the University of Delawarew, was part of a National Science Foundation research coordination network that released a
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Prepare for a remarkable journey into magnificent magnification with “Nanocosmos: Journeys in Electron Space” (Abrams Books, 2025), a mesmerizing new science coffee table book from author, artist, documentarian and visual
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This article was originally published at The Conversation. The publication contributed the article to Space.com’s Expert Voices: Op-Ed & Insights. When I imagine the future of space commerce, the first
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The Elephant Trunk Nebula captured by astrophotographer Terry Hancock (Image credit: Terry Hancock) Astrophotographer Terry Hancock has captured a dramatic view of the star-forming region IC 1396 — also known






