scholarly journals Water and the Interior Structure of Terrestrial Planets and Icy Bodies

Author(s):  
J. Monteux ◽  
G. J. Golabek ◽  
D. C. Rubie ◽  
G. Tobie ◽  
E. D. Young
2018 ◽  
Vol 214 (1) ◽  
Author(s):  
J. Monteux ◽  
G. J. Golabek ◽  
D. C. Rubie ◽  
G. Tobie ◽  
E. D. Young

1998 ◽  
Vol 11 (1) ◽  
pp. 237-238
Author(s):  
J.C. Brandt ◽  
M.F. A’Hearn

The evidence for a major population of small comets (SCs) is summarized in two steps. First, we briefly summarize our previous work. Second, we describe recent work that continues to find SCs. When new capabilities become available that can detect SCs, we expect to find them and this is occurring. At present, their detection is a haphazard process and we advocate a dedicated, optimized search program. We define SCs as those icy bodies (i.e., sublimating bodies) with radius less than 1000 meters. Often the existence of SCs is inferred from effects ascribed to them. These “effects” include: lunar cratering; cratering on Ganymede; excess interplanetary hydrogen; delivery of volatile materials to the terrestrial planets; and a source of fragile bodies entering the Earth’s atmosphere. While some of these indirect methods support the existence of SCs, direct observations are clearly preferred.


1981 ◽  
Vol 1 (7) ◽  
pp. 117-129 ◽  
Author(s):  
V.N. Zharkov ◽  
S.V. Kozlovskaya ◽  
I.Ya. Zasurskii

2010 ◽  
Vol 6 (S276) ◽  
pp. 82-88 ◽  
Author(s):  
Sean N. Raymond ◽  
Philip J. Armitage ◽  
Amaya Moro-Martín ◽  
Mark Booth ◽  
Mark C. Wyatt ◽  
...  

AbstractThe eccentric orbits of the known extrasolar giant planets provide evidence that most planet-forming environments undergo violent dynamical instabilities. Here, we numerically simulate the impact of giant planet instabilities on planetary systems as a whole. We find that populations of inner rocky and outer icy bodies are both shaped by the giant planet dynamics and are naturally correlated. Strong instabilities – those with very eccentric surviving giant planets – completely clear out their inner and outer regions. In contrast, systems with stable or low-mass giant planets form terrestrial planets in their inner regions and outer icy bodies produce dust that is observable as debris disks at mid-infrared wavelengths. Fifteen to twenty percent of old stars are observed to have bright debris disks (at λ ~ 70μm) and we predict that these signpost dynamically calm environments that should contain terrestrial planets.


2005 ◽  
Vol 175 (6) ◽  
pp. 643
Author(s):  
Lev M. Zelenyi ◽  
M.I. Verigin ◽  
A.V. Zakharov ◽  
V.V. Izmodenov ◽  
Aleksandr A. Skal'skii

2000 ◽  
Vol 6 (1) ◽  
pp. 56-63
Author(s):  
K.K. Kamensky ◽  
V.S. Kislyuk ◽  
Ya.S. Yatskiv ◽  
◽  

Sign in / Sign up

Export Citation Format

Share Document