Results 21 to 30 of about 15,866 (198)

Surface Geology of Jupiter’s Trojan Asteroids

open access: yesSpace Science Reviews, 2023
AbstractThe surface geology of Jupiter’s Trojan asteroids is one of the scientific investigations of the NASALucymission. A dedicated Geology Working Group will implement these studies using primarily panchromatic and color imaging data and complement the interpretation of these data with theoretical models, such as collisional evolution models ...
S. Marchi   +3 more
openaire   +1 more source

Near-IR Spectral Observations of the Didymos System: Daily Evolution Before and After the DART Impact Indicates that Dimorphos Originated from Didymos

open access: yesThe Planetary Science Journal, 2023
Ejecta from Dimorphos following the DART mission impact significantly increased the brightness of the Didymos–Dimorphos system, allowing us to examine subsurface material.
David Polishook   +6 more
doaj   +1 more source

Laboratory impact splash experiments to simulate asteroid surfaces [PDF]

open access: yesIcarus, 2020
Granular material that is bound by the low gravity of a small asteroid is mobilized by slow velocity impacts. These splashes generated by impacts might play an important role in sculpting the asteroid's surface. In laboratory experiments we characterize the ejecta generated by spherical 150 $\rm m$ diameter basalt grains impacting a granular bed at 0.
Bogdan, Tabea   +4 more
openaire   +2 more sources

Constraining the Limitations of NEATM-like Models: A Case Study with Near-Earth Asteroid (285263) 1998 QE2

open access: yesThe Planetary Science Journal, 2023
Near-Earth asteroids (NEAs) are a key test bed for investigations into planet formation, asteroid dynamics, and planetary defense initiatives. These studies rely on understanding NEA sizes, albedo distributions, and regolith properties.
Samuel A. Myers   +6 more
doaj   +1 more source

Scaling forces to asteroid surfaces: The role of cohesion

open access: yes, 2010
The scaling of physical forces to the extremely low ambient gravitational acceleration regimes found on the surfaces of small asteroids is performed. Resulting from this, it is found that van der Waals cohesive forces between regolith grains on asteroid ...
Hartzell, C. M.   +3 more
core   +1 more source

OSIRIS-APEX: An OSIRIS-REx Extended Mission to Asteroid Apophis

open access: yesThe Planetary Science Journal, 2023
The Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) spacecraft mission characterized and collected a sample from asteroid (101955) Bennu.
Daniella N. DellaGiustina   +53 more
doaj   +1 more source

A Spectroscopic Comparison of HED Meteorites and V-type Asteroids in the Inner Main Belt [PDF]

open access: yes, 2010
V-type asteroids in the inner Main Belt (a < 2.5 AU) and the HED meteorites are thought to be genetically related to one another as collisional fragments from the surface of the large basaltic asteroid 4 Vesta.
Binzel, Richard   +4 more
core   +2 more sources

Poincar\'e surfaces of section around a 3-D irregular body: The case of asteroid 4179 Toutatis

open access: yes, 2017
In general, small bodies of the solar system, e.g., asteroids and comets, have a very irregular shape. This feature affects significantly the gravitational potential around these irregular bodies, which hinders dynamical studies.
Motta, Gabriel Borderes   +1 more
core   +2 more sources

An Asteroid Lander/Rover for Asteroid Surface Gravity Surveying

open access: yes, 2016
Microsat and nanosat developers have mastered the challenges involved in developing low-cost, high-performance satellite missions in low Earth orbit. Here we describe a proposed small-microsat-scale (~20 kg) planetary exploration mission based on the same design approach used in those LEO missions.
Carroll, Kieran A.   +2 more
openaire   +2 more sources

Simulating the (99942) Apophis Earth Flyby Using a Contact Binary Model

open access: yesThe Planetary Science Journal
This paper investigates the mass shifts of asteroid (99942) Apophis during its 2029 close encounter with Earth, using the contact dynamics method, a type of discrete element method. Unlike previous analyses, we model the asteroid as a contact binary body
Hai-Shuo Wang   +2 more
doaj   +1 more source

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