Abstract
We present Spitzer Space Telescope infrared photometry of a secondary eclipse of the hot Neptune GJ 436 b. The observations were obtained using the 8-μm band of the InfraRed Array Camera (IRAC). The data spanning the predicted time of secondary eclipse show a clear flux decrement with the expected shape and duration. The observed eclipse depth of 0.58 mmag allows us to estimate a blackbody brightness temperature of TP = 717 ± 35 K at 8 μm. We compare this infrared flux measurement to a model of the planetary thermal emission, and show that this model reproduces properly the observed flux decrement. The timing of the secondary eclipse confirms the non-zero orbital eccentricity of the planet, while also increasing its precision (e = 0.14 ± 0.01). Additional new spectroscopic and photometric observations allow us to estimate the rotational period of the star and to assess the potential presence of another planet.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1125-1129 |
| Number of pages | 5 |
| Journal | Astronomy and astrophysics |
| Volume | 475 |
| Issue number | 3 |
| DOIs | |
| State | Published - Dec 2007 |
| Externally published | Yes |
Keywords
- Eclipses
- Infrared: general
- Planetary systems
- Stars: individual: GJ 436
- Techniques: photometric
- Techniques: spectroscopic
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science