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Entering orbit…
Habitability
0/ 100
Uninhabitable
HD 179949 b rendered in TerraForge from its measured mass, orbit and star

HD 179949 b

Also written HD 179949b

Gas Giant90 light years awayFound 2000
Mass
291.00 × Earth
Radius
13.90 × Earth
Gravity
1.51 g
Surface (est.)
1,571 K
Year
3.1 days
From Earth
89.7 ly
Mass
291.00 × Earth
Radius
13.90 × Earth
Gravity
1.51 g
Surface (est.)
1,571 K
Year
3.1 days
From Earth
89.7 ly

HD 179949 system

Type
F-type (White)
Spectral type
F8 V
Temperature
6,168 K
Radius
1.27 ☉
Mass
1.21 ☉
Planets
1
Luminosity
2.00 ☉

Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.

Habitable zone

Star and planets drawn to scale: the star is 10.0 times as wide as HD 179949 b, so only its edge is in view. Orbits spaced as in the star system view.

Estimated: this planet doesn't transit its star, so its size is inferred, not measured

HD 179949 b, from the NASA Exoplanet Archive (found 2000). Measured: 291 Earth masses, 0.0443 AU, a 6168 K F-type star. Composition inferred from a mass of 291 Earths, which is giant territory whatever its 0.11x density suggests, with a day locked to its 3.1-day year, as anything orbiting this close would be.

Surface. No solid surface - thick gaseous envelope with possible rocky core deep within

Gas Giant
Magnetic FieldExtreme Activity
HD 179949 b has 86.0% hydrogen and helium, combined with a mass of 291.0x Earth, which exceeds the gas giant threshold.
Gas giants form when massive cores capture enormous atmospheres of light gases. They typically form beyond the 'frost line' where volatiles can condense.
Classification Criteria:
✓ Hydrogen + Helium: 86.0% (>60% required)✓ Mass: 291.0x Earth (>10x required)

Reading HD 179949 b’s atmosphere

Dominant elements: H, He, O, C, NThis is what a telescope would measure while HD 179949 b crosses in front of its star: starlight passes through the atmosphere and spreads into a rainbow band. Each dark line marks a wavelength the atmosphere absorbed.Every element absorbs its own signature wavelengths — hydrogen always darkens the same two spots, calcium another pair, and so on. Astronomers match the lines in a real spectrum against a library of these signatures to say what an atmosphere is made of, light-years away, without ever visiting. A deeper line generally means more of that element is present.HD 179949 b sits about 90 light-years away, found by the radial velocity method. Most catalogued distances trace back to parallax: as Earth orbits the Sun, a nearby star appears to shift very slightly against the distant background stars, and the size of that shift gives its distance directly.
Habitability ScoreUninhabitable
0
Contributing Factors
temperature0
Inferno world - temperatures exceed all possibility of life
atmosphere30

Hydrogen and helium dominated with trace methane and ammonia

Hydrogen-rich atmosphere typical of gas giants
water15
No solid surface — any water is locked in a supercritical mantle and hot ice, not oceans
magnetic Field100
Magnetic field provides radiation protection
geology40
Extreme volcanic activity may be hazardous
Organic Chemistry80
Core organic elements (CHNO) present
rotation65
Slow rotation - significant day/night temperature variations, but life can adapt

Physical Properties

Mass
291.00x Earth (1.74e+27 kg)
Radius
6.63x Earth (42,219 km)
This planet: 6.63× Earth radiusEarth: 1× (baseline)
Surface Gravity
6.63x Earth (65.0 m/s²)
Surface Temperature
1,571 K (1,298 °C / 2,368 °F)
Rotation Period
74.2 hours/day (slower than Earth)
This planet: 74 h/dayEarth: 24 h/day

Time Dilation

Clocks run 13.7 seconds per year slower than deep space — about 18 minutes over a lifetime

Elemental Composition

A dark ringed planet hanging over the horizon of a rocky moon, its rings lit by a distant sun

New: Stand on Your Moons 🌒

A planet's surface view isn't the only ground any more. Press the surface button on a planet with moons and it asks where to stand: the planet itself, or any moon still in orbit, each tagged with what it became — ocean, ice, carbon, volcanic. Every moon gets its own ground and sky from its own physics: airless rock under a black sky, ice cracked by geysers over a hidden sea, sulfur plains shaking with eruptions, or orange haze you can't see the sun through. And hanging over the horizon, there's the planet you built.

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