lpetrich
Contributor
Or more precisely, some planets have been discovered from transits observed by that satellite. [NASA Exoplanet Archive](https://exoplanetarchive.ipac.caltech.edu/) notes 9 confirmed planets and 482 candidate planets in TESS's data.
Data flows from NASA's TESS Mission, leads to discovery of Saturn-sized planet -- ScienceDaily is about another one. The planet orbits star TOI-197 ("TESS Object of Interest"), and TESS's observations have enabled the discovery of both the planet and some of the star's interior features. The latter is "starquakes", and research into them is "asteroseismology". Some of the articles that I found on this discovery had mixed up the planet transits and the starquake observations, and I was glad to discover that that ScienceDaily did not mix the two up. Once this planet was discovered, its star was observed with a high-resolution spectroscope, and that enabled radial-velocity measurements.
The star has a mass of 1.2 solar masses and a radius of 2.9 solar radii. It is around 5 billion years old, and it has started to move off the main sequence to become a red giant.
The planet has 60 Earth masses and 9 Earth radii, with a density of about 0.4 g/cm^3, a little less than Saturn's, 0.7 g/cm^3. It orbits at about 0.12 AU with a period of 14.3 (Earth) days. It received about 343 times as much light per unit area as the Earth does, implying an equilibrium temperature of about 1300 K.
Turning to the star's oscillations, the most prominent ones are around frequency of 430 microhertz, or an oscillation period of 39 minutes. Their combined amplitude is about 20 parts per million.
The system's distance is 95 parsecs or 310 light years.
Data flows from NASA’s TESS Mission, leads to discovery of Saturn-sized planet • News Service • Iowa State University
[1901.01643] A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS
Data flows from NASA's TESS Mission, leads to discovery of Saturn-sized planet -- ScienceDaily is about another one. The planet orbits star TOI-197 ("TESS Object of Interest"), and TESS's observations have enabled the discovery of both the planet and some of the star's interior features. The latter is "starquakes", and research into them is "asteroseismology". Some of the articles that I found on this discovery had mixed up the planet transits and the starquake observations, and I was glad to discover that that ScienceDaily did not mix the two up. Once this planet was discovered, its star was observed with a high-resolution spectroscope, and that enabled radial-velocity measurements.
The star has a mass of 1.2 solar masses and a radius of 2.9 solar radii. It is around 5 billion years old, and it has started to move off the main sequence to become a red giant.
The planet has 60 Earth masses and 9 Earth radii, with a density of about 0.4 g/cm^3, a little less than Saturn's, 0.7 g/cm^3. It orbits at about 0.12 AU with a period of 14.3 (Earth) days. It received about 343 times as much light per unit area as the Earth does, implying an equilibrium temperature of about 1300 K.
Turning to the star's oscillations, the most prominent ones are around frequency of 430 microhertz, or an oscillation period of 39 minutes. Their combined amplitude is about 20 parts per million.
The system's distance is 95 parsecs or 310 light years.
Data flows from NASA’s TESS Mission, leads to discovery of Saturn-sized planet • News Service • Iowa State University
[1901.01643] A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS