Results 131 to 140 of about 505 (181)

Models and observational predictions of dust traps in protoplanetary discs. [PDF]

Astrophys Space Sci
Pinilla P.
europepmc   +1 more source

The initial solar system abundance of ⁶⁰Fe and early core formation of the first asteroids. [PDF]

Sci Adv
Fang L, Moynier F, Chaussidon M, Limare A, Makhatadze GV, Villeneuve J.   +5 more
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Physicochemical Controls on the Compositions of the Earth and Planets. [PDF]

Space Sci Rev
Sossi PA, Hin RC, Kleine T, Morbidelli A, Nimmo F.   +4 more
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Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]

Nature
Lagrange AM, Wilkinson C, Mâlin M, Boccaletti A, Perrot C, Matrà L, Combes F, Beust H, Rouan D, Chomez A, Milli J, Charnay B, Mazevet S, Flasseur O, Olofsson J, Bayo A, Kral Q, Carter A, Crotts KA, Delorme P, Chauvin G, Thebault P, Rubini P, Kiefer F, Radcliffe A, Mazoyer J, Bodrito T, Stasevic S, Langlois M.   +28 more
europepmc   +1 more source

NASA'S <i>Lucy</i> Mission to Trojan Asteroids: Unraveling the History of the Outer Solar System. [PDF]

Space Sci Rev
Levison HF, Marchi S, Noll KS, Spencer JR, Olkin CB, Statler TS.   +5 more
europepmc   +1 more source

Psyche Mission Description and Design Rationale. [PDF]

Space Sci Rev
Polanskey CA, Elkins-Tanton LT, Bell JF, Alonge EK, Bairstow SH, Binzel RP, Biswas A, Bury L, Cisneros E, Han D, Jun I, Klipstein WM, Lawrence DJ, McCoy TJ, Mastrodemos N, Merayo JMG, Noble SK, Oh DY, Oran R, Ortega CA, Park RS, Peplowski PN, Prettyman TH, Rayman MD, Ream JB, Roatsch T, Weise TM, Wenkert DD, Weiss BP, Zuber MT.   +29 more
europepmc   +1 more source

Instantaneous formation of interstellar minerals and mineral quantum dots. [PDF]

RSC Adv
Roy A, Singh SV, Ramachandran R, Meka JK, Ambresh M, Vijay T, Janardhan P, Jayaram V, Venkatraman V, Das A, Hill H, Bhardwaj A, Mason NJ, Sivaraman B.   +13 more
europepmc   +1 more source

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Planetesimals

2017
Processes governing the evolution of planetesimals are critical to understanding how rocky planets are formed, how water is delivered to them, the origin of planetary atmospheres, how cores and magnetic dynamos develop, and ultimately, which planets have the potential to be habitable.
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Radial Migration of Planetesimals

Astrophysics and Space Science, 1994
Planetesimals orbiting a protostar in a circumstellar disk are affected by gravitational interaction among themselves and by gas drag force due to disk gas. Within the Kyoto model of planetesimal accretion, the migration rate is interpreted as the inverse of the planetary formation time scale. Here, we study time scales of gravitational interaction and
Neuhäuser, R., Feitzinger, J.
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