Results 51 to 60 of about 6,852,218 (267)

The Secular Dynamical Evolution of Binary Asteroid System (65803) Didymos Post-DART

open access: yesThe Planetary Science Journal
The successful impact of NASA’s DART mission with Dimorphos, the secondary body of binary asteroid system (65803) Didymos, altered the attitude, shape, and orbit of Dimorphos.
Rachel H. Cueva   +7 more
doaj   +1 more source

OBSERVED ASTEROID SURFACE AREA IN THE THERMAL INFRARED [PDF]

open access: yesThe Astronomical Journal, 2017
ABSTRACT The rapid accumulation of thermal infrared observations and shape models of asteroids has led to increased interest in thermophysical modeling. Most of these infrared observations are unresolved. We consider what fraction of an asteroid’s surface area contributes the bulk of the emitted thermal flux for two model asteroids of ...
C. R. Nugent   +7 more
openaire   +3 more sources

Q-type asteroids: Possibility of non-fresh weathered surfaces [PDF]

open access: yesNippon Tenmon Gakkai obun kenkyu hokoku, 2019
Itokawa particles, which are samples recovered from the S-complex asteroid 25143 Itokawa by the Hayabusa spacecraft, demonstrate that S-complex asteroids are parent bodies of ordinary chondrite meteorites.
S. Hasegawa   +6 more
semanticscholar   +1 more source

Boulders on asteroid Toutatis as observed by Chang’e-2 [PDF]

open access: yesScientific Reports, 2015
Boulders are ubiquitously found on the surfaces of small rocky bodies in the inner solar system and their spatial and size distributions give insight into the geological evolution and collisional history of the parent bodies. Using images acquired by the
Yun Jiang   +5 more
semanticscholar   +1 more source

Dynamic 3D Simulation of Surface Charging on Rotating Asteroids

open access: yesThe Astrophysical Journal
The surface-charging phenomenon of asteroids, mainly resulting from solar wind plasma and solar radiation, has been extensively studied. However, the influence of the asteroid’s rotation on surface charging is not yet fully understood.
Ronghui Quan, Zhiying Song, Zhigui Liu
doaj   +1 more source

Early evolutionary history of the seed

open access: yesBiological Reviews, EarlyView.
ABSTRACT The seed is an essential stage in the life history of gymnospermous and angiospermous plants, facilitating both their survival and dispersal. We reappraise knowledge of the evolutionary history of the gymnospermous seed, from its origin in the late Devonian through to the well‐known end‐Permian extinctions – an interval encompassing the ...
Richard M. Bateman   +2 more
wiley   +1 more source

Surface Compositions of Trojan Asteroids

open access: yesSpace Science Reviews
AbstractThe Jupiter Trojan asteroids are a key population for understanding the chemical and dynamical evolution of the Solar System. Surface compositions of Trojans, in turn, provide crucial information for reconstructing their histories. NASA’s Lucy mission will soon complete the first spacecraft reconnaissance of this population.
Joshua P. Emery   +8 more
openaire   +2 more sources

Regolith mechanics on Asteroid surfaces

open access: yes, 2017
Introduction: It is very likely that most aster- oids surfaces are covered by a regolith layer. We are focussing on the mechanical properties of such regolith, i.e., a granular material under micro-gravity (µ-g) conditions. Any operations on asteroids that are not remote, need to interact mechanically with the surface material, and for resource ...
Biele, Jens, Ulamec, Stephan
openaire   +2 more sources

Episodes of particle ejection from the surface of the active asteroid (101955) Bennu

open access: yesScience, 2019
Bennu ejects material from its surface Most asteroids appear inert, but remote observations show that a small number experience mass loss from their surfaces. Lauretta and Hergenrother et al.
D. Lauretta   +59 more
semanticscholar   +1 more source

DETECTION OF WATER AND/OR HYDROXYL ON ASTEROID (16) Psyche [PDF]

open access: yes, 2016
In order to search for evidence of hydration on M-type asteroid (16) Psyche, we observed this object in the 3 μm spectral region using the long-wavelength cross-dispersed (LXD: 1.9–4.2 μm) mode of the SpeX spectrograph/imager at the NASA Infrared ...
D. Takir   +4 more
semanticscholar   +1 more source

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