How Scientists Confirmed The Mass Of An Invisible Exoplanet |
That’s especially true of the curious case of Kepler-88 c, which researchers using the Kepler space telescope said was a possible planet due to its effects on the orbit of Kepler-88 b, a planet that goes across the host of its host star. European astronomers just confirmed the Kepler data using the SOPHIE spectrograph at France’s Haute-Provence Observatory.
It’s the first time scientists have successfully used a technique to independently verify a planet’s mass based on what was found from the transit timing variation, or how a planet’s orbit varies from what is expected as it goes across the face of its sun. That means TTV can likely be used as a strong method on its own, advocates say.
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© Elizabeth Howell for Universe Today, 2013. |Permalink |No comment |
Post tags: aix-marseille university, kepler-88, kepler-88 b, kepler-88 c, transit timing variation, university of porto
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