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The Kepler-80 system’s four outermost planets align every month i.e after every 27 days, a new study suggests.
If you want to see a planet align with another in our solar system, you usually have to wait a while. Even the speediest planet, Mercury, takes 88 days to make a circuit around the sun.
But in many alien systems discovered by NASA’s Kepler space telescope, planets are huddled close to their host stars and zoom around it in just a few days. And in one system, Kepler-80, the planets are “synchronized” in such a way that the planets align every month. These planets repeat an alignment every 27 days, returning to the same positions relative to each other, a new study finds.
Kepler-80, a system about 1,100 light-years away, has five known planets. These worlds orbit their star in periods of 1.0, 3.1, 4.6, 7.1 and 9.5 days. Packed tightly around their star, the four outermost planets align every month. These planets return to the same position relative to each other in less than a month, according to the new study. Such a condition is called resonance, and it is one reason the system can stay stable.
Kepler-80 System’s 4 Planets Align Every Month
The study team — led by Mariah MacDonald, who was an undergraduate at Florida Institute of Technology at the time — analyzed Kepler data of the Kepler-80 system. They determined that the four outer planets are all between four and seven times the mass of Earth. The researchers think these worlds are rocky “super-Earths,” though two likely have atmospheres composed mostly of hydrogen and helium. (Earth’s air is primarily nitrogen and oxygen.)
Kepler-80-type configurations actually aren’t all that uncommon. They are called Systems with Tightly- spaced Inner Planets, or STIPs. Hundreds of these STIPs have been found to date. What’s unusual about Kepler-80 is the system’s orbital resonance, which allows the planets to repeat their positions so often. It’s also rare to have a good idea of the composition of four exoplanets in a single system, researchers said.
The new study has been accepted for publication in The Astronomical Journal. You can read a copy of it at the online preprint site Arxiv.org here: http://arxiv.org/abs/1607.07540. Originally published on Space.com.
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