PIA24580: Exoplanet XO-3b Illustration


Exoplanet XO-3b Illustration

Caption:

click here for Figure 1 for PIA24580
Figure 1

Planet XO-3b has an internal source of heat, possibly from tidal heating, which is caused by the squeezing of the planet's interior by the gravity of its parent star. This could be increased by the planet's slightly elliptical orbit (shown on the right), meaning it's more oval-shaped than circular.

Background Info:

The entire body of scientific data collected by Spitzer during its lifetime is available to the public via the Spitzer data archive , housed at the Infrared Science Archive at IPAC at Caltech in Pasadena, California. JPL, a division of Caltech, managed Spitzer mission operations for NASA's Science Mission Directorate in Washington. Science operations were conducted at the Spitzer Science Center at IPAC at Caltech. Spacecraft operations were based at Lockheed Martin Space in Littleton, Colorado.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA.

Cataloging Keywords:

Name Value Additional Values
Target
System
Target Type Exoplanet
Mission Spitzer Space Telescope
Instrument Host Spitzer Space Telescope
Host Type Space Telescope
Instrument Spitzer Space Telescope
Detector
Extra Keywords Color, Infrared, Orbit
Acquisition Date
Release Date 2022-01-13
Date in Caption
Image Credit NASA/JPL-Caltech
Source photojournal.jpl.nasa.gov/catalog/PIA24580
Identifier PIA24580