J u m p t o c o n t e n t
M a i n m e n u
M a i n m e n u
N a v i g a t i o n
● M a i n p a g e ● C o n t e n t s ● C u r r e n t e v e n t s ● R a n d o m a r t i c l e ● A b o u t W i k i p e d i a ● C o n t a c t u s ● D o n a t e
C o n t r i b u t e
● H e l p ● L e a r n t o e d i t ● C o m m u n i t y p o r t a l ● R e c e n t c h a n g e s ● U p l o a d f i l e
S e a r c h
Search
A p p e a r a n c e
● C r e a t e a c c o u n t ● L o g i n
P e r s o n a l t o o l s
● C r e a t e a c c o u n t ● L o g i n
P a g e s f o r l o g g e d o u t e d i t o r s l e a r n m o r e ● C o n t r i b u t i o n s ● T a l k
( T o p )
1 C h a r a c t e r i s t i c s
T o g g l e C h a r a c t e r i s t i c s s u b s e c t i o n
1 . 1 M a s s a n d r a d i u s
1 . 2 O r b i t
2 H o s t s t a r
3 S e e a l s o
4 R e f e r e n c e s
T o g g l e t h e t a b l e o f c o n t e n t s
T O I - 3 2 3 5 b
A d d l a n g u a g e s
A d d l i n k s
● A r t i c l e ● T a l k
E n g l i s h
● R e a d ● E d i t ● V i e w h i s t o r y
T o o l s
T o o l s
A c t i o n s
● R e a d ● E d i t ● V i e w h i s t o r y
G e n e r a l
● W h a t l i n k s h e r e ● R e l a t e d c h a n g e s ● U p l o a d f i l e ● S p e c i a l p a g e s ● P e r m a n e n t l i n k ● P a g e i n f o r m a t i o n ● C i t e t h i s p a g e ● G e t s h o r t e n e d U R L ● D o w n l o a d Q R c o d e ● W i k i d a t a i t e m
P r i n t / e x p o r t
● D o w n l o a d a s P D F ● P r i n t a b l e v e r s i o n
A p p e a r a n c e
F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
TOI-3235 b is a gas giant exoplanet found 237 light-years away from Earth.[2] transit method .[2]
Characteristics
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Mass and radius
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TOI-3235 b was discovered by the transit method. The exoplanet's mass is ± 0.025 M J ± 0.04 M J semi-major axis is 0.02709± 0.00046 AU ± 19 Kelvin [3]
Orbit
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TOI-3235 b has a smaller orbit than Mercury . The exoplanet's orbit is 2.6 days, which is similar to the orbital period of Gliese 436 b and has an inclination of ± 0.046 Degree (angle)
Host star
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The host star of the exoplanet is TOI-3235, a M-type main sequence star (red dwarf) that is not visible to the naked eye from Earth with a apparent magnitude of 14.5.[4] ± 0.003 M ☉ ± 0.0018 R ☉ ± 68 Kelvin [3] Centaurus .[4] [a]
See also
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References
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^ a b "TOI-3235b" . Exoplanet Exploration: Planets Beyond our Solar System . Retrieved 2024-01-14 .
^ a b "The Extrasolar Planet Encyclopaedia — TOI-3235 b" . Extrasolar Planets Encyclopaedia
^ a b "★ TOI 3235" . Stellar Catalog . Retrieved 2024-01-14 .
^ Based on right ascension and declination provided in the source, and placed in this website .
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=TOI-3235_b&oldid=1195622890 " C a t e g o r i e s : ● E x o p l a n e t s d i s c o v e r e d i n 2 0 2 3 ● T r a n s i t i n g e x o p l a n e t s ● G i a n t p l a n e t s H i d d e n c a t e g o r i e s : ● A r t i c l e s w i t h s h o r t d e s c r i p t i o n ● S h o r t d e s c r i p t i o n m a t c h e s W i k i d a t a
● T h i s p a g e w a s l a s t e d i t e d o n 1 4 J a n u a r y 2 0 2 4 , a t 1 6 : 3 6 ( U T C ) . ● T e x t i s a v a i l a b l e u n d e r t h e C r e a t i v e C o m m o n s A t t r i b u t i o n - S h a r e A l i k e L i c e n s e 4 . 0 ;
a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n . ● P r i v a c y p o l i c y ● A b o u t W i k i p e d i a ● D i s c l a i m e r s ● C o n t a c t W i k i p e d i a ● C o d e o f C o n d u c t ● D e v e l o p e r s ● S t a t i s t i c s ● C o o k i e s t a t e m e n t ● M o b i l e v i e w
