Extrasolar Carbon Planets

Astrophysics, abstract
astro-ph/0504214

From: Sara Seager [view email]
Date: Fri, 8 Apr 2005 20:12:45 GMT   (36kb)

Extrasolar Carbon Planets
Authors: Marc J. Kuchner (Princeton), S. Seager (Carnegie/DTM)
Comments: 17 pages, 2 figures, submitted to ApJL

We suggest that some extrasolar planets <~ 60 Earth masses will form substantially from silicon carbide and other carbon compounds. Pulsar planets and low-mass white dwarf planets are especially good candidate members of this new class of planets, but these objects could also conceivably form around stars like the Sun. This planet-formation pathway requires only a factor of two local enhancement of the protoplanetary disk's C/O ratio above solar, a condition that pileups of carbonaceous grains may create in ordinary protoplanetary disks. Hot, Neptune-mass carbon planets should show a significant paucity of water vapor in their spectra compared to hot planets with solar abundances. Cooler, less massive carbon planets may show hydrocarbon-rich spectra and tar-covered surfaces. The high sublimation temperatures of diamond, SiC, and other carbon compounds could protect these planets from carbon depletion at high temperatures.

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