Ultra-short period planet | Wikipedia audio article
Channel: wikipedia tts
Date: 29/05/2019

This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Hot_Jupiter


00:00:39 1 General characteristics
00:02:50 2 Formation and evolution
00:03:15 2.1 Migration
00:04:43 2.2 In situ
00:06:27 2.3 Atmospheric loss
00:07:17 3 Terrestrial planets in systems with hot Jupiters
00:09:05 4 Retrograde orbit
00:10:25 5 Ultra-short period planets
00:11:39 6 Puffy planets
00:13:12 7 Moons
00:14:01 8 Hot Jupiters around red giants
00:15:09 9 Star-Planet Interactions
00:16:59 10 See also



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Voice name: en-AU-Wavenet-A


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SUMMARY
=======
Hot Jupiters are a class of gas giant exoplanets that are inferred to be physically similar to Jupiter but that have very short orbital periods (P10 days). The close proximity to their stars and high surface-atmosphere temperatures resulted in the moniker "hot Jupiters".Hot Jupiters are the easiest extrasolar planets to detect via the radial-velocity method, because the oscillations they induce in their parent stars' motion are relatively large and rapid compared to those of other known types of planets. One of the best-known hot Jupiters is 51 Pegasi b. Discovered in 1995, it was the first extrasolar planet found orbiting a Sun-like star. 51 Pegasi b has an orbital period of about 4 days.