Results 201 to 210 of about 20,127 (260)

The Origins & Reservoirs of Exocomets. [PDF]

Space Sci Rev
Bannister M, Pfalzner S, Pearce T, Mustill AJ, Klahr H, Nomura H, Ohashi N, Kokotanekova R, Marino S, Bodewits D, Marschall R, Seligman DZ, Jones GH, Veras D.   +13 more
europepmc   +1 more source

Photometry and Models of Seven Main-Belt Asteroids

Jun Tian, Haibin Zhao, Bin Li, Yongxiong Zhang, Jian Chen, L. Elenin, Xiaoping Lu   +6 more
openalex   +1 more source

Author Correction: The geology and evolution of the Near-Earth binary asteroid system (65803) Didymos. [PDF]

Nat Commun
Barnouin O, Ballouz RL, Marchi S, Vincent JB, Agrusa H, Zhang Y, Ernst CM, Pajola M, Tusberti F, Lucchetti A, Daly RT, Palmer E, Walsh KJ, Michel P, Sunshine JM, Rizos JL, Farnham TL, Richardson DC, Parro LM, Murdoch N, Robin CQ, Hirabayashi M, Kahout T, Asphaug E, Raducan SD, Jutzi M, Ferrari F, Hasselmann PHA, CampoBagatin A, Chabot NL, Li JY, Cheng AF, Nolan MC, Stickle AM, Karatekin O, Dotto E, Della Corte V, Mazzotta Epifani E, Rossi A, Gai I, Deshapriya JDP, Bertini I, Zinzi A, Trigo-Rodriguez JM, Beccarelli J, Ivanovski SL, Brucato JR, Poggiali G, Zanotti G, Amoroso M, Capannolo A, Cremonese G, Dall'Ora M, Ieva S, Impresario G, Lavagn M, Modenini D, Palumbo P, Perna D, Pirrotta S, Tortora P, Zannoni M, Rivkin AS.   +62 more
europepmc   +1 more source

Rapid Dynamical Evolution in the Arjuna Asteroid Belt: Apollo 2022 RD ₂ Goes from Mini-moon to Virtual Impactor in About 40 yr

C. de la Fuente Marcos, R. de la Fuente Marcos   +1 more
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Dynamics around small irregularly shaped objects modeled as a mass dipole. [PDF]

Sci Rep
Abozaid AA, Radwan M, Ibrahim AH, Bakry A.   +3 more
europepmc   +1 more source

Transport of dust across the Solar System: Constraints on the spatial origin of individual micrometeorites from cosmic-ray exposure. [PDF]

Philos Trans A Math Phys Eng Sci
Feige J, Airo A, Berger D, Brückner D, Gärtner A, Genge M, Leya I, Habibi Marekani F, Hecht L, Klingner N, Lachner J, Li X, Merchel S, Nissen J, Patzer ABC, Peterson S, Schropp A, Sager C, Suttle MD, Trappitsch R, Weinhold J.   +20 more
europepmc   +1 more source

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Physical study of outer belt asteroids

Advances in Space Research, 1991
Abstract Located in the proximity of Jovian resonances, the outer belt asteroids are kept from interacting with other asteroids and are likely to represent a population of primitive bodies. The systematic investigation of the physical properties of these objects and the subsequent understanding of their nature and origin, will have a direct ...
Gonano, M., di Martino, M., Mottola, S., Neukum, G.   +3 more
openaire   +3 more sources

Solar Electric Propulsion Asteroid Belt Mission

Journal of Spacecraft and Rockets, 1970
This paper presents the major results from a study of an unmanned asteroid belt probe powered by solar electric propulsion (SEP) and launched by an Atlas/Centaur or a Titan IIIC. The SEP comprises roll-out solar cell arrays, mercury electron-bombardment ion thrusters, and modular solid-state power-conditioning equipment. With a 10-kw solar array (rated
D. MACPHERSON, J. MOLITOR, L. SCHWAIGER, J. SHOLLENBERGER, JR.   +3 more
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Compositional Structure of the Asteroid Belt

Science, 1982
The distribution of compositional types among the asteroids is found to vary systematically with heliocentric distance. Seven distinct peaks in the relative proportion of the compositional types E, R, S, M, F, C, P, and D are found from 1.8 to 5.2 astronomical units.
J, Gradie, E, Tedesco
openaire   +2 more sources

Stable Chaos in the Asteroid Belt☆

Icarus, 1997
Abstract Most asteroids are characterized by positive Lyapounov Characteristic Exponents (LCE), which means that their orbits are chaotic. Indeed, the striking fact is that for many of them the maximum LCE is very large, with a corresponding Lyapounov time shorter (often much shorter) than 100,000 years, as we report in this work.
MILANI COMPARETTI, ANDREA, NOBILI, ANNA MARIA, KNEZEVIC, ZORAN   +2 more
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