51 Pegasi itself isn't an exoplanet, it's a Sun-like Star. But it does have an Exoplanet orbiting it, 51 Pegasi b (informally named Bellerophon.).
The first confirmed exoplanet is called 51 Pegasi b. It was discovered on October 6th 1995 by Michel Mayor and Didier Queloz. Note: 51 Pegasi or 51 Pegasi a is the parent star.
51 Pegasi B is an exoplanet orbiting a sun like star called 51 Pegasi.S Ori 70 - Is still not confirmed. It might be a brown dwarf, but it could be an exoplanet.
51 Pegasi is approximately 50.9 light-years away from Earth. It is a star located in the constellation of Pegasus and is known for hosting the first exoplanet discovered orbiting a main-sequence star.
As of now, there are no confirmed moons orbiting 51 Pegasi b. This exoplanet, discovered in 1995, is a gas giant located about 50 light-years away in the constellation Pegasus. While some scientists speculate that exoplanets could have moons, observational evidence for such moons around 51 Pegasi b has not yet been found.
51 Pegasi was discovered by astronomers Michel Mayor and Didier Queloz in 1995. They identified it as the first Sun-like star known to host an exoplanet, which was later named 51 Pegasi b. This discovery marked a significant milestone in the field of astronomy, opening up new avenues in the search for exoplanets. Their work earned them the Nobel Prize in Physics in 2019.
The star they were observing, 51 Pegasi, moved back and forth only very slightly. Therefore, they knew the invisible object could not have enough mass to be a star. They deduced that it must be a planet.
There are hundreds of "exoplanets" (in orbit around stars other than Sol), but these don't have proper names, just designations. The usual convention is to add a lowercase letter to the designation of the star, so an object orbiting 51 Pegasi would be 51 Pegasi a, the next object 51 Pegasi b, and so on.
The sun of the exoplanet Gliese 581 is a red dwarf star, emitting redder light than our Sun. It is cooler and less massive than our Sun, making it dimmer and emitting less heat and light. Therefore, the sun of Planet Gliese is not as hot as the sun of Earth.
The discovery of 51 Pegasi b was the first confirmed exoplanet orbiting a sun-like star, challenging the previously-held belief that such planets were rare. It prompted a reassessment of our understanding of planetary formation and the diversity of planetary systems beyond our own, sparking new research and exploration in the field of exoplanets. This discovery fundamentally shifted the perception of our place in the universe by demonstrating that planetary systems were more varied and complex than previously thought.
It's much closer to its star than Jupiter is to the Sun.
51 Pegasi is a G-type main-sequence star, similar to our Sun, and it has a yellowish-white color. Its luminosity is approximately 0.95 times that of the Sun, indicating it emits slightly less light. This makes it a relatively bright star in its vicinity, but not exceptionally luminous compared to other stars in the galaxy.
At least 28 planets were found in 2008, all of them exoplanets (i.e. planets oribiting stars other than the Sun). Exoplanets are generally named as follows: Technical star name + lower case letter denoting the order in which the planets are discovered around that star (starting with "b" because "A" stands for the star itself). For instance 51 Pegasi b means the first planet discovered orbiting the star 51 Pegasi.