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Kepler 469
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Star Kepler 469

Subgiant Kepler 469 is located 3029 light years away from the Sun. It is a single star of spectral class G0IV, that has 106 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
3029 light years
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Kepler 469

Subgiant
Spectral class: G0IV

Location +

Ascension iconRight ascension: 19h 49m 54.217s
Declination iconDeclination: 41° 6' 51.385'' (northern hemisphere)
Parallax iconParallax: 1.077
Distance iconSun distance: 3,029.203 ly | 928.8 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 106 % M Sun
| 1110 M Jupiter
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Star mass
Mass of the star Kepler 469 is 1.06 solar masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
radius icon
Size: 219 % R Sun
| 21.8 R Jupiter
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Star size
Radius of the star Kepler 469 is 2.19 solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide
temperature icon
Temperature: 5846 K | 1.01 T Sun
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Star temperature
Surface temperature of Kepler 469 is 5846 K, which is 101 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide
time icon
Age: 5.37 billions years | 1.17 Sun
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Star age
Star Kepler 469 is 5.37 billion years old, which is about 1.17 of the Sun's age.

The age of a star tells us how long it has been shining since it formed. Knowing a star’s age helps astronomers understand its life stage, how it has changed over time, and what will happen to it in the future... icon More about Star age in StellarGuide

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
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Kepler 469 system structure

 Kepler 469
Kepler 469 b 0.02 AU 0.7 R⊕ 0.9 days

More about Kepler 469

Star Kepler 469 is is approximately 2 times bigger than the Sun and temperature on its surface is around 5846 K (5573 °C), which is about 101 % of Sun's temperature.
       Kepler 469 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
KIC 5897826, KOI-126, Gaia DR3 2076863875880496256
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External sources
gaia icon
Gaia database (Gaia DR3 2076863875880496256)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Kepler 469 system from the Sun?

The Kepler 469 system is 3029 light years or 928.8 parsecs from the Sun.

What galaxy is the Kepler 469 star in?

The Kepler 469 is in the Milky Way galaxy just like the Sun.

How many stars are in the Kepler 469 system?

The Kepler 469 is a single star, there are no other known stars in the system.

What type of star is the Kepler 469?

The star Kepler 469 is a Subgiant star.

What temperature is star Kepler 469?

The star Kepler 469 has an effective temperature of 5846 K. Find out more about the temperature of stars in Stellar guide
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
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