Structure of the Secretory Compartments in Goblet Cells in the Colon and Small Intestine. [PDF]
Mironov AA +6 more
europepmc +1 more source
Visibility of lunar craters during the LEM final approach phase
I. Saulietis
openalex +1 more source
Anatomical Study and CT Scan of the Scleral Ring in the Little Owl (Athene noctua)
The scleral ring in Athene noctua predominantly consists of 15 quadrilateral ossicles, with a rare anatomical variation of 16 ossicles observed unilaterally in one specimen. Structural Morphology: The ring displays a distinct bipartite architecture, featuring an anterior tubular segment with a near‐circular cross‐section and a posterior funnel‐shaped ...
Omid Zehtabvar +6 more
wiley +1 more source
Space weathering effects in Bennu asteroid samples. [PDF]
Keller LP +21 more
europepmc +1 more source
Effect of Boulder‐Size Distributions on Thermally Derived Rock Abundances on the Moon
Abstract Rock abundance, defined as the surface's fractional area covered by rocks, is used to characterize the Moon's regolith, decipher its impact history, and assess potential landing sites. By definition, it should be agnostic to rock‐size distributions. However, it has been suggested that rock abundances, derived from surface temperatures measured
Brian Amaro +4 more
wiley +1 more source
YOLOv8-LCNET: An Improved YOLOv8 Automatic Crater Detection Algorithm and Application in the Chang'e-6 Landing Area. [PDF]
Nan J +9 more
europepmc +1 more source
A Temporally Consistent Spatial Gradient in Methane Ebullition From a Eutrophic Lake
Abstract Gas bubble emission (ebullition) from lake sediment is a prominent source of the greenhouse gas methane (CH4) to the atmosphere, but the stochastic nature of bubble release and thus high variability in space and time makes the estimation of lake CH4 ebullition challenging.
S. Moras +3 more
wiley +1 more source
Recent aqueous alteration associated to sedimentary volcanism on Mars. [PDF]
Pineau M +7 more
europepmc +1 more source
Abstract The Lunar Trailblazer smallsat mission High‐resolution Volatiles and Minerals Moon Mapper (HVM3) science instrument was designed to acquire targeted spectral image cubes of the lunar surface at visible to shortwave infrared (VSWIR) wavelengths (0.6–3.6 μm) in an effort to understand the distribution, abundance, and form (OH, H2O, ice) of lunar
Angela M. Dapremont +13 more
wiley +1 more source
NASA'S <i>Lucy</i> Mission to Trojan Asteroids: Unraveling the History of the Outer Solar System. [PDF]
Levison HF +5 more
europepmc +1 more source

