Doppler cross-correlation spectroscopy as a path to the detection of Earth-like planets
In the middle of the 20th century, a paradigm shift appeared concerning the expected frequency of planetary systems in the galaxy ...a shift induced by the observation of the rotational velocities of low main sequence stars (Struve 1952)!At the same time, Fellgett (1955) proposed to concentrate the...
Saved in:
Main Author: | Mayor, Michel |
---|---|
Format: | Article |
Language: | English |
Published: |
Académie des sciences
2023-06-01
|
Series: | Comptes Rendus. Physique |
Subjects: | |
Online Access: | https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.153/ |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Revised Masses for Low-density Planets Orbiting the Disordered M-dwarf System TOI-1266
by: Dakotah Tyler, et al.
Published: (2025-01-01) -
An HST Transmission Spectrum of the Closest M Dwarf Transiting Rocky Planet LTT 1445Ab
by: Katherine A. Bennett, et al.
Published: (2025-01-01) -
Exoplanet Occurrence Rate with Age for FGK Stars in Kepler
by: Maryum Sayeed, et al.
Published: (2025-01-01) -
Stellar X-Ray Variability and Planetary Evolution in the DS Tucanae System
by: George W. King, et al.
Published: (2025-01-01) -
Planetary Mass Determinations from a Simplified Photodynamical Model—Application to the Complete Kepler Dataset
by: Aviv Ofir, et al.
Published: (2025-01-01)