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PDS 111
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Star PDS 111

T Tauri star PDS 111 is located 517 light years away from the Sun. It is a single star of spectral class G2, that has typically about 100 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
517 light years

PDS 111

Spectral class: G2

Location +

Ascension iconRight ascension: 5h 24m 37.265s
Declination iconDeclination: -8° 42' 1.913'' (equatorial region)
Parallax iconParallax: 6.314
Distance iconSun distance: 516.596 ly | 158.4 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: 80 % M Sun
| 880 M Jupiter
 (estimate)
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Star mass
The mass of the star PDS 111 is unknown. Based on its other characteristics, it is estimated to be about 80 % of the Sun’s mass.

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: 152 % R Sun
| 15.1 R Jupiter
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Star size
Radius of the star PDS 111 is 1.52 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: 5900 K | 1.02 T Sun
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Star temperature
Surface temperature of PDS 111 is 5900 K, which is 102 % 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: 0.016 billions years | 0 Sun
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Star age
Star PDS 111 is 0.016 billion years old, which is about 0 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
luminosity icon
Luminosity: 2.52 L Sun
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Star luminosity
Luminosity is the total amount of energy a star gives off every second. Think of it as the star’s true brightness — not just how bright it looks from Earth. This is important because some stars may appear dim simply because they are far away, not because they’re actually faint... icon More about Star luminosity in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 10
Magnitude iconAbsolute magnitude (V): 4
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
More about PDS 111
Star PDS 111 is is approximately 52 % bigger than the Sun and temperature on its surface is around 5900 K (5627 °C), which is about 102 % of Sun's temperature.
       PDS 111 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia DR3 3014890093437477120
External sources
gaia icon
Gaia database (Gaia DR3 3014890093437477120)
Archive from the Gaia mission

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Estimated values
icon Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.
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