This article is from the 2025 Technical Update. The NESC has invested significant time and resources to better understand composite overwrapped pressure vessels (COPV) performance and more importantly, how these complex, high-pressure
This article is from the 2025 Technical Update. The NESC has invested significant time and resources to better understand composite overwrapped pressure vessels (COPV) performance and more importantly, how these complex, high-pressure
Experimental set-up of the MMS-2 incubation. (a) One side of a two compartment Petri dish was filled with 1 g of heat-treated MMS-2; the other side contained 10 mL of Milli-Q
This article is from the 2025 Technical Update. The NESC’s Thermal Control & Protection Technical Discipline Team (TDT) is a resource providing subject matter expertise in active and passive thermal
NASA/JPL-Caltech/Univ. of Arizona NASA’s Mars Reconnaissance Orbiter (MRO) captures a detailed view of a relatively fresh crater in this image released on June 3, 2015. The crater has a sharp
Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on
(top) Schematic of the novel region extraction (NRE) pipeline. NREs cascade a class-agnostic region proposal system with full-image novelty detection and can be trained like traditional reconstruction-based novelty detectors. (bottom)
(a) CORALS engineering test unit. (b) Schematic diagram of Fig. 1a illustrating key subsystems and components. (c) Ion optics simulation using SIMION® 8.1, showing a cut plane of the instrument.
Lower-triangular Pearson correlation matrix of the final feature set used in this study. Each cell shows the Pearson correlation coefficient between a pair of planetary or stellar properties, with the
WASHINGTON — Space mobility company Impulse Space has opened a Colorado facility to support development of its spacecraft. The company, based in Southern California, said March 10 it opened a
Spectra of NEOs with (potential) 3 μm absorption features. (A) Spectrum of (161989) Cacus as observed on 2022 September 3 and 4. (B) (756998) 2024 CR9 as observed on 2024






