Gigantic exoplanet ring system around J1407b much larger, heavier than Saturn’s, the first of its kind to be found outside our solar system.
Image © Ron Miller
Astronomers at the Leiden Observatory, The Netherlands, and the University of Rochester, USA, have discovered that the ring system that they see eclipse the very young Sun-like star J1407 is of enormous proportions, much larger and heavier than the ring system of Saturn. The ring system was discovered in 2012 by a team led by Rochester’s Eric Mamajek.
A new analysis of the data, led by Leiden’s Matthew Kenworthy, shows that the ring system consists of over 30 rings, each of them tens of millions of kilometers in diameter. Furthermore, they found gaps in the rings, which indicate that satellites (“exomoons”) may have formed.
“The details that we see in the light curve are incredible. The eclipse lasted for several weeks, but you see rapid changes on time scales of tens of minutes as a result of fine structures in the rings. The star is much too far away to observe the rings directly, but we could make a detailed model based on the rapid brightness variations in the star light passing through the ring system. If we could replace Saturn’s rings with the rings around J1407b, they would be easily visible at night and be many times larger than the full moon.”
Co-author Eric Mamajek, professor of physics and astronomy at the University of Rochester, said:
“This planet is much larger than Jupiter or Saturn, and its ring system is roughly 200 times larger than Saturn’s rings are today. You could think of it as kind of a super Saturn.”
Astronomers expect that the rings will become thinner in the next several million years and eventually disappear as satellites form from the material in the disks.
Computer model that fits the light curve of the star J1407 seen in SuperWASP data in 2007. The model is described in Kenworthy and Mamajek (2015).
Source University of Rochester
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