Recent advancements in the radial velocity (RV) method for detecting exoplanets have brought scientists closer to the threshold required to identify Earth-mass and potentially habitable planets around Sun-like stars.
To address this issue, a team of researchers utilized a partially automated method to analyze spectral lines in observations of the young, active star ϵ Eridani from the high-precision NEID spectrograph.
Publisher: CityLife
Date: 2023-11-21T01:53:17 00:00
Author: Mampho Brescia
Reference: (Read more) Visit Source
No comments:
Post a Comment