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TOI-4138 b, the Glossary

Index TOI-4138 b

TOI-4138 b is a transiting exoplanet orbiting the G-type subgiant TOI-4138 1,674 light years away in the northern circumpolar constellation Ursa Minor.[1]

Table of Contents

  1. 19 relations: Apparent magnitude, Astronomical transit, Circumpolar star, Day, Doppler spectroscopy, Effective temperature, Exoplanet, Hot Jupiter, Julian day, Jupiter, Light-year, Mercury (planet), Orbital inclination, Orbital period, Solar mass, Subgiant, Sun, Transiting Exoplanet Survey Satellite, Ursa Minor.

  2. Exoplanets discovered by TESS
  3. Exoplanets discovered in 2021

Apparent magnitude

Apparent magnitude is a measure of the brightness of a star or other astronomical object.

See TOI-4138 b and Apparent magnitude

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 TOI-4138 b and Astronomical transit

Circumpolar star

A circumpolar star is a star that, as viewed from a given latitude on Earth, never sets below the horizon due to its apparent proximity to one of the celestial poles.

See TOI-4138 b and Circumpolar star

Day

A day is the time period of a full rotation of the Earth with respect to the Sun.

See TOI-4138 b and Day

Doppler spectroscopy

Doppler spectroscopy (also known as the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star.

See TOI-4138 b and Doppler spectroscopy

Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation.

See TOI-4138 b and Effective temperature

Exoplanet

An exoplanet or extrasolar planet is a planet outside the Solar System.

See TOI-4138 b and Exoplanet

Hot Jupiter

Hot Jupiters (sometimes called hot Saturns) are a class of gas giant exoplanets that are inferred to be physically similar to Jupiter but that have very short orbital periods (. TOI-4138 b and hot Jupiter are hot Jupiters.

See TOI-4138 b and Hot Jupiter

Julian day

The Julian day is the continuous count of days since the beginning of the Julian period, and is used primarily by astronomers, and in software for easily calculating elapsed days between two events (e.g. food production date and sell by date).

See TOI-4138 b and Julian day

Jupiter

Jupiter is the fifth planet from the Sun and the largest in the Solar System.

See TOI-4138 b and Jupiter

Light-year

A light-year, alternatively spelled light year (ly or lyr), is a unit of length used to express astronomical distances and is equal to exactly 9,460,730,472,580.8 km (Scientific notation: 9.4607304725808 × 1012 km), which is approximately 5.88 trillion mi.

See TOI-4138 b and Light-year

Mercury (planet)

Mercury is the first planet from the Sun and the smallest in the Solar System.

See TOI-4138 b and Mercury (planet)

Orbital inclination

Orbital inclination measures the tilt of an object's orbit around a celestial body.

See TOI-4138 b and Orbital inclination

Orbital period

The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object.

See TOI-4138 b and Orbital period

Solar mass

The solar mass is a standard unit of mass in astronomy, equal to approximately.

See TOI-4138 b and Solar mass

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.

See TOI-4138 b and Subgiant

Sun

The Sun is the star at the center of the Solar System.

See TOI-4138 b and Sun

Transiting Exoplanet Survey Satellite

Transiting Exoplanet Survey Satellite (TESS) is a space telescope for NASA's Explorer program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission.

See TOI-4138 b and Transiting Exoplanet Survey Satellite

Ursa Minor

Ursa Minor (Latin: 'Lesser Bear', contrasting with Ursa Major), also known as the Little Bear, is a constellation located in the far northern sky.

See TOI-4138 b and Ursa Minor

See also

Exoplanets discovered by TESS

Exoplanets discovered in 2021

References

[1] https://en.wikipedia.org/wiki/TOI-4138_b

Also known as TIC 257060897b, TOI-4138b.