do not follow here

Star TIC 400799224

Binary star TIC 400799224 is located 2566 light years away from the Sun. It consists of a yellow-white star and a yellow star. For now, there are no known exoplanets in this star system.
Sun distance
2566 light years

TIC 400799224 A

Yellow-White star

Location

Ascension iconRight ascension: 11h 9m 58.186s
Declination iconDeclination: -66° 45' 14.91'' (southern hemisphere)
Parallax iconParallax: 0
Distance iconSun distance: 2566 ly | 786.7 pc

Basic characteristic

icon weight
Mass: 179 % M Sun | 1875 M Jupiter
radius icon
Size: 247 % R Sun | 24.6 R Jupiter
temperature iconTemperature: 5829 K | 1.01 T Sun
time iconAge: 0.005 billions years | 0 Sun
luminosity iconLuminosity: 6.32 L Sun

1 exoplanet

TIC 400799224 A dust belt n/a -

Photometry

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
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

TIC 400799224 B

Yellow star

Basic characteristic

icon weight
Mass: 161 % M Sun | 1687 M Jupiter
radius icon
Size: 202 % R Sun | 20.1 R Jupiter
temperature iconTemperature: 5465 K | 0.95 T Sun
time iconAge: 0.00553 billions years | 0 Sun
luminosity iconLuminosity: 3.25 L Sun
(No known exoplanets yet)
More about TIC 400799224
      TIC 400799224 can be found in southern celestial hemisphere. 
Other designations of this star
Gaia EDR3 5238414793089292160, 2MASS 11095818-6645149, WISEA J110958.16-664514.8
External sources
icon study
Mysterious Dust-emitting Object Orbiting TIC 400799224
Scientific study, Submitted: 03. 10. 2021
News from this star system
Article image:

Weird behavior of star TIC 40079922 might be caused by a dust emitting object or broken up exoplanet

Astronomers led by Brian Powell found a strange object in the data from the space telescope TESS. It is a star with designation TIC 400799224, which periodically changes its brightness. While the period is always 19,77 days, the dip in brightness varies greatly. Astronomers argue that this behavior might be caused by a dust-emitting object or maybe a broken up asteroid or exoplanet.

Get your next news from nearby stars
This is a new project, and partly still in development. There will be soon more information and functions. We would love your support on social media.
Living Future: Nearby stars
Follow @LIVINGfUTUREcz