HD 189733 - Planetary System

Planetary System

HD 189733 A has one known planet, designated HD 189733 b, a gaseous giant 13% larger than Jupiter close enough to complete an orbit every two days. Using spectrometry it was found in 2007 that this planet contains significant amounts of water vapour. This planet is the second extrasolar planet where definitive evidence for water has been found.

The chemical signature of water vapour was detected in the atmosphere of this planet. Although HD 189733b with atmospheric temperatures rising above 1,000 °C (1,830 °F) is far from being habitable, this finding increases the likelihood that water, an essential component of life, would be found on a more Earth-like planet in the future.

Astronomers have created a rough map of HD 189733b's cloud-top features using data from the Spitzer infrared space telescope.

Although Spitzer could not resolve the planet into a disk, by measuring changes as the planet rotated, the team created a simple longitudinal map. That is, they measured the planet's brightness in a series of pole-to-pole strips across the planet's visible cloud-tops, then assembled those strips into an overall picture.

Probably due to strong winds, the hottest point on the planet seems to be "offset by about 30 degrees longitudinally" from the substellar point ("high noon").

In late 2008, the spectral signature of carbon dioxide was found in HD 189733b's atmosphere.

The HD 189733 system
Companion
Mass Semimajor axis
Orbital period
Eccentricity Radius
b 1.13 ± 0.03 MJ 0.03099 ± 0.0006 2.21857 ± 0.00002 0.0010 ± 0.0002

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