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Planetary system · 2 known planets · Cetus

LHS 1140

Its star: above the horizon after darkHighest after dark 00:49 · south · 23°
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LHS 1140N ↑ E ← · 36° FIELD

Where is LHS 1140?

Times for LondonChange city

Look south, about 23° up at 00:49 in Cetus.

Rises
20:04
Highest
00:48
Sets
05:31
Best after dark
00:49 · 23°

Can I see LHS 1140?

No. The planets of LHS 1140 can’t be seen with the eye, binoculars or any amateur telescope: they are lost in their star’s light. What you can do is point toward the star.

From London tonight, the star LHS 1140 is above the horizon after dark. It’s highest after dark at 00:49, in the south at 23°.

Why is LHS 1140 interesting?

LHS 1140 has 2 known planets, discovered between 2017 and 2018 by the primary transit method.

One of them is close to Earth’s size or mass, based on the catalog values.

What can you see?

Eyes

Direction only

Not visible.

Binoculars

Not visible.

Telescope

The star is around magnitude 14 and needs a large amateur telescope and a detailed chart. The planets themselves can’t be seen with any backyard telescope.

What you’re likely to see, not what a space telescope photographs.

About

LHS 1140 is a quiet red dwarf about 41 light-years away in Cetus. Its planet LHS 1140 b is a super-Earth, larger and heavier than our planet, orbiting in the habitable zone every 25 days.

Because it passes in front of its star and is relatively close, it is one of the best targets for studying a potentially habitable world. Early James Webb Space Telescope observations hint that it may have an atmosphere, but the results are tentative.

LHS 1140 b is about 1.7 times Earth’s width and several times its mass. Its density suggests it may contain a large fraction of water, which could make it an ocean world or a frozen snowball.

Its star has only about a fifth of the Sun’s mass, and a second, inner planet, LHS 1140 c, orbits closer and is too hot for liquid water.

The planets were found by watching the star dim slightly as they passed in front of it.

The LHS 1140 system

Known planets of LHS 1140 (catalog values from exoplanet.eu)
PlanetMassRadiusOrbitFrom starFoundMethod
LHS 1140 c1.81 M⊕1.28 R⊕3.78 days0.0268 AU2018Primary Transit
LHS 1140 b6.99 M⊕1.73 R⊕24.7 days0.0936 AU2017Primary Transit

M⊕ / R⊕ = Earth masses / radii; M♃ / R♃ = Jupiter. Masses from radial velocity are often minimum masses. Data: The Extrasolar Planets Encyclopaedia, exoplanet.eu (CC BY 4.0).

Questions

Could LHS 1140 b have water?
Possibly. Its density suggests it could hold a lot of water, but this is not confirmed.

Sources: The Extrasolar Planets Encyclopaedia (CC BY 4.0); star chart: Wikidata (CC0). Positions computed for your place and time with astronomy-engine. Data & Licences