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KELT-18 b

Hot Jupiter Ursa Major

KELT-18 b is a hot Jupiter orbiting the F4 V star KELT-18 in the constellation Ursa Major. It lies about 1,048 light-years from Earth and was discovered in 2017 using the transit method.

17.60×Earth radius
375×Earth mass
2.9 dOrbital period
2,085 KEquilibrium temp.
0.05Earth similarity
1,048 lyDistance
2017Discovered

How Big Is KELT-18 b?

Earth1.00 R⊕KELT-18 b17.60 R⊕Jupiter11.21 R⊕
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KELT-18 b has a radius of 17.60 times that of Earth, or 1.57 times the radius of Jupiter. Its mass is 375 times that of Earth, giving it a density of 0.38 g/cm³ — closer to gas planets like Jupiter (1.33 g/cm³).

Is KELT-18 b in the Habitable Zone?

KELT-18 b orbits inside the inner edge of the habitable zone of KELT-18. So close to its star, surface conditions are far too hot for liquid water.

KELT-18 b
Too hot Optimistic habitable zone Conservative habitable zone Too cold

Habitable zone of KELT-18: 1.814–4.201 AU (conservative: 2.298–3.983 AU), per Kopparapu et al. (2014). Earth orbits the Sun at 1 AU.

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Temperature on KELT-18 b

The equilibrium temperature of KELT-18 b is about 2,085 K (1,812 °C) — hot enough to melt many metals. This estimate ignores any atmosphere, which could change surface temperatures dramatically — Earth's greenhouse effect adds about 33 °C. It receives 3,152 times the stellar energy that Earth gets from the Sun.

Orbit and Year Length

A year on KELT-18 b — one full orbit around KELT-18 — lasts 2.87 Earth days, shorter than Mercury's 88-day year. It orbits at an average distance of 0.046 AU — closer to its star than Mercury is to the Sun.

How Was KELT-18 b Discovered?

KELT-18 b was discovered in 2017 using the transit method, with observations from KELT-North.

The transit method watches a star for the tiny, regular dip in brightness that occurs when a planet crosses in front of it. The depth and timing of these dips reveal the planet's size and orbital period.

How Far Away Is KELT-18 b?

KELT-18 b is 1,048.2 light-years (321.4 parsecs) from Earth. Light arriving here tonight left the planet about 1,048 years ago. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 18,448,320 years to make the journey.

Earth Similarity Index

The Earth Similarity Index (ESI) scores how physically similar a planet is to Earth, from 0 to 1, based on radius, density, escape velocity and surface temperature. KELT-18 b scores 0.05, ranking #5,257 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.

The Host Star: KELT-18

KELT-18 b belongs to a system of 2 stars; it orbits KELT-18.

KELT-18

Spectral type
F4 V
Surface temperature
6,670 K (Sun: 5,772 K)
Mass
1.52 M☉
Radius
1.91 R☉
Luminosity
6.4999 L☉
Age
1.9 billion years (Sun: 4.6)

Planetary System

KELT-18 b is the only planet known to orbit KELT-18 so far.

KELT-18 b — Complete Data

Radius17.598 Earth radii (1.570 Jupiter radii)
Mass375.04 Earth masses (1.180 Jupiter masses)
Density0.38 g/cm³ (Earth: 5.51)
Orbital period2.87 days
Orbital distance0.046 AU
Equilibrium temperature2,085 K (1,812 °C)
Stellar irradiation3,152.00× Earth
Earth Similarity Index0.05
Distance from Earth1,048.2 light-years (321.4 parsecs)
ConstellationUrsa Major
Discovery methodTransit
Discovery facilityKELT-North
Discovery year2017

Data: NASA Exoplanet Archive, last updated 2017-04-24. Earth Similarity Index: PHL @ UPR Arecibo.

Frequently Asked Questions About KELT-18 b

Is KELT-18 b habitable?

No — KELT-18 b orbits too close to its star and is too hot for liquid water to exist on its surface.

How far away is KELT-18 b?

KELT-18 b is about 1,048 light-years from Earth in the constellation Ursa Major. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 18,448,320 years to get there.

How big is KELT-18 b compared to Earth?

KELT-18 b has 17.60 times the radius of Earth and about 375 times its mass.

How long is a year on KELT-18 b?

One orbit around KELT-18 takes 2.9 Earth days — short enough that 127 of its years would fit into one Earth year.

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