Zobrazeno 1 - 4
of 4
pro vyhledávání: '"C. T. Unterborn"'
Autor:
J. G. Schulze, Ji Wang, J. A. Johnson, B. S. Gaudi, R. Rodriguez Martinez, C. T. Unterborn, W. R. Panero
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 71 (2024)
Using mass–radius composition models, small planets ( R ≲ 2 R _⊕ ) are typically classified into three types: iron-rich, nominally Earth-like, and those with solid/liquid water and/or atmosphere. These classes are generally expected to be varia
Externí odkaz:
https://doaj.org/article/770426f28a364f4c837bbee3c6fb4838
Autor:
C. T. Unterborn, S. J. Desch, J. Haldemann, A. Lorenzo, J. G. Schulze, N. R. Hinkel, W. R. Panero
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 1, p 42 (2023)
The two primary observable quantities of an exoplanet—its mass and radius—alone are not sufficient to probe a rocky exoplanet’s interior composition and mineralogy. To overcome this, host-star abundances of the primary planet-building elements
Externí odkaz:
https://doaj.org/article/d4bea8f241fe4398a2baef849fb14805
Autor:
C. T. Unterborn, S. J. Desch, J. Haldemann, A. Lorenzo, J. G. Schulze, N. R. Hinkel, W. R. Panero
The two primary observable quantities of an exoplanet--its mass and radius--alone are not sufficient to probe a rocky exoplanet's interior composition and mineralogy. To overcome this, host-star abundances of the primary planet-building elements (Mg,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de7deff8d6a067ac7436d86f57574870
Publikováno v:
Astrophysical Journal; 3/1/2016, Vol. 819 Issue 1, p1-1, 1p