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Star HAT-P-62

Yellow star HAT-P-62 is located 1151 light years away from the Sun. It is a single star, that has 102 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
1151 light years

HAT-P-62

Location +

Ascension iconRight ascension: 4h 58m 1.000s
Declination iconDeclination: 48° 18' 4.000'' (northern hemisphere)
Parallax iconParallax: 2.834
Distance iconSun distance: 1,150.836 ly | 352.8 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: 102.3 % M Sun
| 1072 M Jupiter
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Star mass
Mass of the star HAT-P-62 is 1.023 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: 117 % R Sun
| 11.6 R Jupiter
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Star size
Radius of the star HAT-P-62 is 1.17 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: 5629 K | 0.97 T Sun
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Star temperature
Surface temperature of HAT-P-62 is 5629 K, which is 97 % 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: 8.1 billions years | 1.76 Sun
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Star age
Star HAT-P-62 is 8.1 billion years old, which is about 1.76 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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HAT-P-62 system structure

HAT-P-62
HAT-P-62 b 0.04 AU 241.9 M⊕ 12 R⊕ 2.6 days

More about HAT-P-62

Star HAT-P-62 is is approximately 17 % bigger than the Sun and temperature on its surface is around 5629 K (5356 °C), which is about 97 % of Sun's temperature.
       HAT-P-62 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
Gaia DR3 255397142179844224
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Frequently Asked Questions

How far is the HAT-P-62 system from the Sun?

The HAT-P-62 system is 1151 light years or 352.8 parsecs from the Sun.

What galaxy is the HAT-P-62 star in?

The HAT-P-62 is in the Milky Way galaxy just like the Sun.

How many stars are in the HAT-P-62 system?

The HAT-P-62 is a single star, there are no other known stars in the system.

What type of star is the HAT-P-62?

The star HAT-P-62 is a Yellow star star.

What temperature is star HAT-P-62?

The star HAT-P-62 has an effective temperature of 5629 K. Find out more about the temperature of stars in Stellar guide
Class of stars Yellow star
Sun-like stars belong mainly to spectral type G and are commonly called yellow dwarfs. They have surface temperatures of roughly 5,300–6,000 K (about 5,000–5,700 °C), giving them a slightly yellow-white appearance. With masses typically between about 0.8 and 1.1 times that of the Sun, they sit between hotter, more massive white stars and cooler orange and red stars on the main sequence. The Sun itself is a standard G2V star and serves as the benchmark for understanding the structure and behavior of this stellar class.

These stars generate energy by fusing hydrogen into helium in their cores through the proton–proton chain. Their total lifetimes on the main sequence are around 10 billion years, during which their brightness slowly increases. After exhausting hydrogen in their cores, Sun-like stars expand into red giants, shed their outer layers to form planetary nebulae, and eventually leave behind dense white dwarfs. Many known exoplanet systems orbit Sun-like stars, making them key targets in the search for potentially habitable worlds.
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