The gas
giant exoplanet orbits the binary red dwarfs at a distance of 300 million miles — approximately the distance of the solar system's asteroid belt from the sun.
SPHERE's main goal is to find and characterise
giant exoplanets orbiting nearby stars by direct imaging [1].
SPHERE's primary task is to discover and study
giant exoplanets orbiting nearby stars using direct imaging.
Not exact matches
In the 1990s the first discovered
exoplanets (planets
orbiting other stars) were Jupiter - like
giants, betrayed by the slight gravitational wobbles in the motion of their parent stars.
Researchers expect to find water on many planets outside the solar system, called
exoplanets, including Jupiter - size gas
giants such as HD 189733 b and HD 209458 b, which
orbits a different star.
The first
exoplanets found were gas
giants orbiting close to their stars — a study suggests they could be built from collisions of several smaller planets
Something strange is a-brewing on upsilon Andromedae b. Astronomers have classified the
exoplanet,
orbiting a sun - like star about 44 light - years away, as a hot Jupiter — a gas
giant circling so close to its parent sun that its atmosphere is boiling away.
To date, all
exoplanets discovered in
orbit around double stars are gas
giants, similar to Jupiter, and are thought to form in the icy regions of their systems.
They hope their technique will eventually produce weather reports for gas
giants orbiting distant stars and, one day, rocky
exoplanets similar to our own.
Most of the first
exoplanets found were hot Jupiters: gas
giants that
orbit close to their stars.
Many of the
exoplanets we see are Jupiter - like gas
giants orbiting close to their star.
According to a NASA announcement on Friday, «TESS will use an array of telescopes to perform an all - sky survey to discover transiting
exoplanets ranging from Earth - sized to gas
giants, in
orbit around the nearest and brightest stars in the sky.
I'm still holding out for the news that reads: «Second Earth Found» -[this
exoplanet] will have all the right ingredients:
orbit its star inside the habitable zone, spectroscopic analysis will reveal a nitrogen - rich atmosphere, evidence of water, roughly the same mass as our planet and it will belong in a system with a couple of gas
giants shepherding the outer system.
Tidal interactions between close - in, gas -
giant exoplanets and their host star should cause the
orbits of the planets to decay.
Young stars that are from a few million to one billion years old and appear to have a disk of dust and debris
orbiting them may be the best place to look for
giant exoplanets.
We underscore the significance of long - term ground - based monitoring of hot stars and space - based targeting of hot stars with the Transiting
Exoplanet Survey Satellite (TESS) to search for inflated
giants in longer - period
orbits.
When researchers observed star systems containing debris disks with
giant exoplanets in distant
orbits, they noted that the star systems had similar dual dust disks analogous to the Solar System's two zones — the asteroid belt (between Mars and Jupiter) and the Kuiper Belt (beyond the
orbit of Neptune).
The project, led by principal investigator George Ricker, a senior research scientist at MKI, will use an array of wide - field cameras to perform an all - sky survey to discover transiting
exoplanets, ranging from Earth - sized planets to gas
giants, in
orbit around the brightest stars in the sun's neighborhood.
The project, led by principal investigator George Ricker, a senior research scientist at the MIT Kavli Institute for Astrophysics and Space Research (MKI) will use an array of wide - field cameras to perform an all - sky survey to discover transiting
exoplanets, ranging from Earth - sized planets to gas
giants, in
orbit around the brightest stars in the sun's neighborhood.
So far the direct detection has only been able to show
giant exoplanets, several times larger than Jupiter and
orbiting at great distances from their stars.
Again the difficulty lies in detecting small
exoplanets at far
orbits, since
giant exoplanets and close
orbits exert much larger gravitational pulls over the star and create easily visible oscillations.
So, if other star systems contain gas
giant exoplanets, it stands to reason that they would have the same effect on bodies
orbiting close to their star.
A more recently announced
exoplanet, Kepler - 453b, is also a circumbinary and a gas
giant, though its
orbit within its star's habitable zone means any moons it might have could be hospitable to life.