Related Experiment Video
Updated: May 8, 2026

Biochemical and High Throughput Microscopic Assessment of Fat Mass in Caenorhabditis Elegans
Published on: March 30, 2013
A transiting giant planet with a temperature between 250 K and 430 K
H J Deeg1, C Moutou, A Erikson
1Instituto de Astrofísica de Canarias, C. Via Lactea S/N, E-38205 La Laguna, Tenerife, Spain. hdeeg@iac.es
Researchers discovered CoRoT-9b, a temperate exoplanet with a large orbit. Its characteristics align with standard planetary evolution models, offering new insights into gas giant composition.
Area of Science:
- Astronomy and Astrophysics
- Exoplanetary Science
Background:
- Over 400 exoplanets have been discovered, with about 70 exhibiting transiting behavior.
- Transiting exoplanets allow for detailed parameter derivation and atmospheric studies.
- Previous discoveries often focused on short-period planets, including terrestrial ones like CoRoT-7b.
Purpose of the Study:
- To report transit observations of the exoplanet CoRoT-9b.
- To characterize CoRoT-9b's orbital parameters and temperature.
- To compare CoRoT-9b's properties with existing planetary evolution models.
Main Methods:
- Transit observations of CoRoT-9b were conducted.
- Orbital period, eccentricity, and periastron distance were determined.
- Photospheric temperature was estimated based on orbital and stellar properties.
Main Results:
- CoRoT-9b orbits a solar-like star with a period of 95.274 days and low eccentricity (0.11 +/- 0.04).
- It possesses the largest periastron distance (0.36 AU) among known transiting planets.
- The planet's estimated photospheric temperature ranges from 250 to 430 K, indicating a temperate climate.
- CoRoT-9b's size is not significantly affected by tidal heating, unlike shorter-period planets.
Conclusions:
- CoRoT-9b's properties are consistent with standard planetary evolution models.
- Its inferred interior composition is similar to that of Jupiter and Saturn.
- This discovery provides a unique case study for understanding temperate exoplanets with wide orbits.
Related Concept Videos
Acceleration due to Gravity on Other Planets
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Schwarzschild Radius and Event Horizon
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Increased Body Temperature
Radiation: Applications
The average...
Atomic Spectroscopy: Effects of Temperature
At thermal equilibrium, the relative populations of excited and ground state atoms can be estimated using the Maxwell–Boltzmann distribution. For example, an increase in temperature from...
Diversity of Archaea IV

