On the Emergent Spectra of Hot Protoplanet Collision Afterglows
We explore the appearance of terrestrial planets in formation by studying the emergent spectra of hot molten protoplanets during their collisional formation. While such collisions are rare, the surfaces of these bodies may remain hot at temperatures of 1000-3000 K for up to millions of years during...
Main Authors: | Miller-Ricci, Eliza, Meyer, Michael R., Seager, Sara, Elkins Tanton, Linda T. |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2012
|
Online Access: | http://hdl.handle.net/1721.1/74030 https://orcid.org/0000-0003-4008-1098 https://orcid.org/0000-0002-6892-6948 |
Similar Items
-
Effects of Stellar Flux on Tidally Locked Terrestrial Planets: Degree-1 Mantle Convection and Local Magma Ponds
by: Gelman, S. E., et al.
Published: (2012) -
A water budget dichotomy of rocky protoplanets from 26Al-heating
by: Lichtenberg, T, et al.
Published: (2018) -
Direct imaging of molten protoplanets in nearby young stellar associations
by: Bonati, I, et al.
Published: (2019) -
An organic afterglow protheranostic nanoassembly
by: He, Shasha, et al.
Published: (2019) -
Protoplanets with core masses below the critical mass fill in their
Roche lobe
by: Terquem, C, et al.
Published: (2011)