Assessing the Impact of H2O and CH4 Opacity Data in Exoplanetary Atmospheres: Laboratory Measurements and Radiative Transfer Modeling Approaches
abstract: One strategic objective of the National Aeronautics and Space Administration (NASA) is to find life on distant worlds. Current and future missions either space telescopes or Earth-based observatories are frequently used to collect information through the detection of...
Other Authors: | Gharib-Nezhad, Ehsan (Author) |
---|---|
Format: | Doctoral Thesis |
Language: | English |
Published: |
2019
|
Subjects: | |
Online Access: | http://hdl.handle.net/2286/R.I.54982 |
Similar Items
-
The Detection and Characterization of Extrasolar Planets
by: Ken Rice
Published: (2014-09-01) -
Analytic Expressions for the Detectability of Exoplanets in Radial Velocity, Astrometric, and Transit Surveys
by: Mogren, Karen Nicole
Published: (2012) -
Numerical exploration of the probability of capture into the 3:1 mean motion resonance
by: Chan, Ka-ho., et al.
Published: (2013) -
New model for the 5-20 cm wavelength opacity of ammonia pressure-broadened by methane under jovian conditions based on laboratory measurements
by: Chinsomboon, Garrett
Published: (2013) -
Microlensing Searches for Exoplanets
by: Yiannis Tsapras
Published: (2018-09-01)