What it’s like to stand here
Kepler-325 b
weight
≈ 1.04 g
sun
18.9× wider
sky
warm white

Illustration computed from this world’s measured and derived values, not a photograph.

Sub-Neptune

Kepler-325 b

Transit: spotted by the tiny, repeating dip in its star’s light each time the planet crosses in front of it.

Kepler-325
host star
2.91 R⊕
radius
8.80 M⊕
mass · estimated from radius
4.5 days
orbital period
744°C (1371°F)
avg temp
What it's like to stand here
≈ 1.04 g
your weight (mass estimated from size)
4.5 days
one year, in Earth time
18.9× wider
how big its sun looks vs ours
warm white
midday sky tint
1.0×
how high you could jump vs Earth
likely
likely tidally locked: probably eternal day on one side, night on the other
How long to get there · 2,685 ly away
Jet airliner
3.2 billion years
dies en route1000-yr cryo: fails
Parker Solar Probethe fastest craft ever built
4.2 million years
dies en route1000-yr cryo: fails
Light speed
2,685 years
dies en route1000-yr cryo: fails
Warp 10
3 years
arrives, just older
Folding spacetime
instant
arrives thriving
Size vs Earth
EarthKepler-325 b is 2.9× the width of Earth
Explore from here · roam the neighborhood
Host star
Kepler-325
5752 K host star · 3 planets
Explore →

Zoom out: star → system → (soon) galaxy arm, host black hole, and a real image of the host galaxy.

Can you see it tonight? · observe
FAINT — LARGE TELESCOPE NEEDED
Host-star brightnessmag 15.2
ConstellationCygnus
To see the host star10"+ (250 mm) telescope, dark sky
Gear bridge

Matched telescope & eyepiece recommendations are coming. Any product links will carry a clear affiliate disclosure.

Illustration generated from Kepler-325 b's confirmed parameters, not a photograph.