NameDimidiumLatin for half: about half Jupiter's mass[5]
About the image. Drawn as a glowing gas giant very close to its yellow star. 51 Pegasi b has never been seen and does not pass in front of its star, so even its size is calculated; the colours are imagined.
23×as wide as our Sun looks from Earth
520×the light Earth gets
No ground: the view from the cloud tops
The sky from 51 Pegasi b
51 Pegasi would look 23× as wide as the Sun does from Earth, and the planet gets 520× as much light as Earth gets.
Its colour comes from its surface temperature of 5 761 K (5 490 °C); the Sun's is about 5 772 K (5 500 °C).
How fast 51 Pegasi b spins is unknown, so the length of its day is too.
Apparent size = star radius ÷ orbit; light = size² × (temperature ÷ 5 772 K)⁴. Both from the values on this page. The landscape is imagined.
On 6 October 1995, at a conference in Florence, two Swiss astronomers, Michel Mayor and Didier Queloz, announced a planet around 51 Pegasi, a Sun-like star about 50 light-years away. It was the first planet ever found around an ordinary star like the Sun. Twenty-four years later it won them the Nobel Prize in Physics.
A wobble in a star
The planet itself has never been seen. Mayor and Queloz detected it through its pull on the star. As a planet orbits, the star swings in a small circle in response, moving slightly towards us and then away, and that motion shifts the colour of its light back and forth. In spring 1994 they had started using a new spectrograph at the Haute-Provence Observatory in France that could measure stellar speeds to 10 or 15 metres per second. 51 Pegasi was swinging by about 59 metres per second, regularly, every 4.23 days.
Nobody expected it
The result made little sense at the time. Jupiter-sized planets were thought to form far from their stars, where it is cold enough for ice, and to take years to complete an orbit. This one had at least half Jupiter’s mass and circled its star in four days, at 0.052 AU, about a seventh of Mercury’s distance from the Sun. Almost no one believed it at first. Then Geoffrey Marcy and Paul Butler in the United States confirmed the wobble, and a new kind of planet, the hot Jupiter, had to be explained. The answer that emerged was migration: giant planets can form far out and then move inward.
First, but not quite the very first
51 Pegasi b was not the first planet found beyond the Solar System. In 1992 Aleksander Wolszczan and Dale Frail had found planets around a pulsar, the remains of an exploded star. But it was the first around a star like the Sun, and the Nobel committee gave Mayor and Queloz half of the 2019 prize “for the discovery of an exoplanet orbiting a solar-type star”.
In 2015 the planet and its star were given names proposed from Switzerland, in a public vote run by the International Astronomical Union: the star became Helvetios and the planet Dimidium, Latin for half, because it has about half Jupiter’s mass.
Half a Jupiter, more or less
Because the planet does not pass in front of its star, its size has never been measured, and the wobble method alone gives only a minimum mass, about 0.47 Jupiters. In 2017 astronomers detected water vapour in its atmosphere by its signature in the starlight. In 2026 measurements with the CRIRES+ instrument on ESO’s Very Large Telescope confirmed the water, worked out how the orbit is tilted, and put the planet’s true mass at about 0.61 Jupiters, higher than earlier estimates. A 2015 claim to have seen light reflected from the planet has not held up: later studies found it reflects very little light at all.
Its orbit, to scale
51 Pegasi b goes around once every 4.2 days, at 0.052 AU from its star. The whole view is tiny on Solar System scale: Mercury orbits the Sun about 7 times farther out than the outermost orbit shown here.
Earth days passing: 0
How hot is it?
Earth (average)288 K · 15 °C
Water boils373 K · 100 °C
Venus surface737 K · 464 °C
Iron melts1 811 K · 1 540 °C
Sun's surface5 772 K · 5 500 °C
51 Pegasi b1 329 K · 1 060 °C
51 Pegasi b: equilibrium temperature (calculated). Logarithmic scale from 100 K to 10 000 K. Reference values: NASA, IAU.
How long to get there?
51 Pegasi b is about 50.4 light-years away.
Light299 792 km/s50 years
Breakthrough Starshotplanned light sail, 20% of light speed252 years
Parker Solar Probefastest spacecraft so far, 192 km/s78 695 years
Voyager 1leaving the Solar System, 17 km/s888 795 years
At Voyager 1's speed the trip would take about 11 110 human lifetimes of 80 years. Bars are on a logarithmic scale. Speeds: NASA, Breakthrough Initiatives.
Gallery
A glowing yellow star on the left and, right beside it, a giant planet banded in dark red and orange, an impression of 51 Pegasi b orbiting very close to its star. AI-generated painting.A sea of dark red and orange clouds stretching to a curved horizon, with a glaring yellow-white star rising above it, an impression of the view above the clouds of 51 Pegasi b. AI-generated painting.51 Pegasi b, 3D artist's impression, rendered from the interactive model.51 Pegasi b, 3D artist's impression, from another angle, rendered from the interactive model.51 Pegasi b, 3D artist's impression, close-up, rendered from the interactive model.
Timeline
1995Michel Mayor and Didier Queloz announce the planet on 6 October in Florence.
2015The IAU names the planet Dimidium and its star Helvetios.
2017Water vapour is detected in its atmosphere.
2019Mayor and Queloz share the Nobel Prize in Physics, announced on 8 October.
2026CRIRES+ measurements put its true mass at about 0.61 Jupiters.
Questions people ask
Was 51 Pegasi b the first exoplanet?
No, but it was the first found around a Sun-like star. Planets around the pulsar PSR B1257+12 were reported in 1992.
Why is 51 Pegasi b called Dimidium?
Because dimidium is Latin for half: the planet has about half Jupiter's mass.
Can you see 51 Pegasi?
Yes, but only with the naked eye under really dark skies. The planet itself has never been seen.