Table of Contents
9 relations: Astronomical transit, Day, K-type main-sequence star, Kelvin, Lyra, Metallicity, Subgiant, Sun, Transit-timing variation.
Astronomical transit
In astronomy, a transit (or astronomical transit) is the passage of a celestial body directly between a larger body and the observer.
See Kepler-410 and Astronomical transit
Day
A day is the time period of a full rotation of the Earth with respect to the Sun.
K-type main-sequence star
A K-type main-sequence star, also referred to as a K-type dwarf, or orange dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow/white G-type main-sequence stars. Kepler-410 and k-type main-sequence star are k-type main-sequence stars.
See Kepler-410 and K-type main-sequence star
Kelvin
The kelvin, symbol K, is the base unit of measurement for temperature in the International System of Units (SI).
Lyra
paren, from λύρα; pronounced) is a small constellation. It is one of the 48 listed by the 2nd century astronomer Ptolemy, and is one of the modern 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence is sometimes referred to as Vultur Cadens or Aquila Cadens ("Falling Vulture" or "Falling Eagle"), respectively.
Metallicity
In astronomy, metallicity is the abundance of elements present in an object that are heavier than hydrogen and helium.
See Kepler-410 and Metallicity
Subgiant
A subgiant is a star that is brighter than a normal main-sequence star of the same spectral class, but not as bright as giant stars.
Sun
The Sun is the star at the center of the Solar System.
Transit-timing variation
Transit-timing variation is a method for detecting exoplanets by observing variations in the timing of a transit.
See Kepler-410 and Transit-timing variation
References
Also known as HD 175289, Kepler-410 Ab, Kepler-410Ab.