Kepler-45b
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Kepler-45, formerly known as KOI-254, is a star in the northern constellation of Cygnus. It is located at the
celestial coordinates Astronomical coordinate systems are organized arrangements for specifying positions of satellites, planets, stars, galaxies, and other celestial objects relative to physical reference points available to a situated observer (e.g. the true hor ...
: right ascension , declination . With an
apparent visual magnitude Apparent magnitude () is a measure of the brightness of a star or other astronomical object observed from Earth. An object's apparent magnitude depends on its intrinsic luminosity, its distance from Earth, and any extinction of the object's lig ...
of 16.88, this star is too faint to be seen with the naked eye. The star is exhibiting strong
starspot Starspots are stellar phenomena, so-named by analogy with sunspots. Spots as small as sunspots have not been detected on other stars, as they would cause undetectably small fluctuations in brightness. The commonly observed starspots are in gene ...
activity, with 4.1% of its surface covered by starspots.


Planetary system

The "Hot Jupiter" class planet Kepler-45b, discovered in February 2011, is unusually massive for the M-class parent star. Its orbit is aligned within 11 degrees of rotational axis of the star. The planet is strongly suspected to have optically thick rings, because planetary shadow appears to be elongated.Revealing peculiar exoplanetary shadows from transit light curves
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See also

* NGTS-1b


References

{{Stars of Cygnus Cygnus (constellation) M-type main-sequence stars
254 Year 254 ( CCLIV) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar. At the time, it was known as the Year of the Consulship of Valerianus and Gallienus (or, less frequently, year 1007 ''Ab urbe ...
Planetary transit variables Planetary systems with one confirmed planet J19312949+4103513