Results 131 to 140 of about 3,518 (157)

Chaotic exchange of solid material between planetary systems: implications for lithopanspermia. [PDF]

Astrobiology, 2012
Belbruno E, Moro-Martín A, Malhotra R, Savransky D.   +3 more
europepmc   +1 more source

Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]

Space Sci Rev
Dickers MD, Mifsud DV, Mason NJ, Fantuzzi F.   +3 more
europepmc   +1 more source

The Dimorphos ejecta plume properties revealed by LICIACube. [PDF]

Nature
Dotto E, Deshapriya JDP, Gai I, Hasselmann PH, Mazzotta Epifani E, Poggiali G, Rossi A, Zanotti G, Zinzi A, Bertini I, Brucato JR, Dall'Ora M, Della Corte V, Ivanovski SL, Lucchetti A, Pajola M, Amoroso M, Barnouin O, Campo Bagatin A, Capannolo A, Caporali S, Ceresoli M, Chabot NL, Cheng AF, Cremonese G, Fahnestock EG, Farnham TL, Ferrari F, Gomez Casajus L, Gramigna E, Hirabayashi M, Ieva S, Impresario G, Jutzi M, Lasagni Manghi R, Lavagna M, Li JY, Lombardo M, Modenini D, Palumbo P, Perna D, Pirrotta S, Raducan SD, Richardson DC, Rivkin AS, Stickle AM, Sunshine JM, Tortora P, Tusberti F, Zannoni M.   +49 more
europepmc   +1 more source

Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons. [PDF]

Space Sci Rev
Rhoden AR, Ferguson SN, Bottke W, Castillo-Rogez JC, Martin E, Bland M, Kirchoff M, Zannoni M, Rambaux N, Salmon J.   +9 more
europepmc   +1 more source

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Investigating Possible Spindown of Arrokoth by Collisions with Small Classical Kuiper Belt Objects

Introduction: The New Horizons flyby of Arrokoth revealed an ancient, contact binary planetesimal [1,2]. Arrokoth’s both lobes’ respective principal axes are aligned within a few degrees [2], and such configuration suggests a co-orbiting Arrokoth before the coalescence of its two lobes [3].
Xiaochen Mao, William McKinnon, Kelsi Singer, James Keane, Stuart Robbins, Paul Schenk, Jeffrey Moore, Alan Stern, Harold Weaver, John Spencer, Catherine Olkin, the New Horizons Science Team   +11 more
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The absolute magnitude distribution of cold classical Kuiper belt objects

2016
We report measurements of the low inclination component of the main Kuiper Belt showing a size freqency distribution very steep for sizes larger than H_r ~ 6.5-7.0 and then a flattening to shallower slope that is still steeper than the collisional equilibrium slope.The Outer Solar System Origins Survey (OSSOS) is ongoing and is expected to detect over ...
Petit, Jean-Marc, Bannister, Michele T., Alexandersen, Mike, Chen, Ying-Tung, Gladman, Brett, Gwyn, Stephen, Kavelaars, Jj, Volk, Kathryn   +7 more
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TNOs are Cool: Analysis of Classical Kuiper Belt Objects from Herschel Space Observatory Data

2012
We present results from the sample analysis of classical Kuiper belt objects (CKBO) observed within the open time key program "TNOs are Cool" [Muller et al. 2009, Earth, Moon, Planets 105] of Herschel Space Observatory. About half of this sample was published in Vilenius et al.
Vilenius, E., Kiss, C., Mommert, M., Müller, T., Santos-Sanz, P., Pal, A., Stansberry, J., Mueller, M., Peixinho, N., Fornasier, S., Lellouch, E., Delsanti, A., Thirouin, A., Duffard, R., Ortiz, J.   +14 more
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Analysis of classical Kuiper-belt objects and Haumea collisional family from the Herschel and Spitzer observations

2014
We have analyzed space-based data at far-IR wavelengths in order to determine physical properties of Kuiper-belt objects (KBOs), also known as transneptunian objects (TNO), in the dynamical class of classical Kuiper-belt objects (CKBO). This dynamical class also contains most of the Haumea family members, the only known collisional family among TNOs ...
Vilenius, E., Stansberry, J., Müller, T., Kiss, C., Mommert, M., Mueller, M., Santos-Sanz, P., Thirouin, A., Lellouch, E., Pal, A., Peixinho, N., Fornasier, S.   +11 more
openaire   +1 more source

Sublimation of ices during the early evolution of Kuiper belt objects

Monthly Notices of the Royal Astronomical Society, 2023
Dina Prialnik
exaly