A relatively
small planet orbiting a star not far from Earth may be made mostly of water, new observations show.
The instrument makes it possible to detect very
small planets orbiting those stars.
Not exact matches
This is the first time
planets have been observed
orbiting ultra-cool dwarves — though scientists had suspected that such
stars could host
small solar systems.
The
planets orbit an «ultracool dwarf,» a
star much
smaller and cooler than the sun, but still possibly warm enough to allow for liquid water on the surfaces of at least two of the
planets.
After a lot of time on a
small planet orbiting a minor
star at the outskirts of a nondescript spiral galaxy, out of those billions of billions of
planets, had the right conditions (right energy and matter flux, etc) for biology to emerge from chemistry.
Both
planets are many hundreds of light - years away and
orbit stars smaller and dimmer than our sun.
Astronomers conducting a galactic census of
planets in the Milky Way now suspect most of the universe's habitable real estate exists on worlds
orbiting red dwarf
stars, which are
smaller but far more numerous than
stars like our Sun.
«It will put special emphasis on
stars smaller and cooler than the sun, because any
planets orbiting such
stars will be easier to detect, confirm and characterize.
Small, rocky
planets like Mercury, Venus, Earth, and Mars would
orbit close to the
star.
Several other super-Earths have been identified in systems much like our solar system, with
small planets closer to the
star and giants in the outer
orbits.
«It shows that astronomers are working their best to optimize techniques to work on
smaller and
smaller planets, and that nature has once again delivered on a fascinating
planet orbiting a bright nearby
star.»
Boss has recently proposed a similar effect to explain the discovery of two gas giants and two so - called super-Earths, or big rocky
planets, each
orbiting a
small red dwarf
star.
Surface temperatures on Proxima b, a
small planet orbiting the dim red
star nearest to Earth, depend on the
planet's spin and the makeup of its atmosphere.
The goal of this work that I did with Berkeley astronomer Andrew Howard was to measure the fraction of
stars that have
small planets in close
orbits.
The standard approach of researching exoplanets, or
planets that
orbit distant
stars, has entailed studying
small numbers of objects to determine if they have the right gases in the appropriate quantities and ratios to indicate the existence of life.
In May 2016, members of the Belgian TRAPPIST team announced their
small telescope had turned up three potentially habitable
planets orbiting a
star just 40 light - years away.
The catalyst for this epochal transition is Proxima b, a newfound
small planet orbiting Proxima Centauri, which at just over four light - years away is the
star nearest to our solar system.
The
planets won't be just like Earth — they'll be bigger, and
orbiting smaller stars — but we'll find them.
The
planet, 51 Pegasi b, was half as massive as Jupiter, but its 4 - day
orbit was impossibly close to the
star, far
smaller than the 88 - day
orbit of Mercury.
In space, above our atmosphere,
stars do not twinkle; in space a telescope is also beyond day and night and can thus stare at the same
star for weeks on end, gradually teasing from its light the barely perceptible but regular flickers caused by a
small orbiting planet.
This scenario naturally produces a planetary system just like our own:
small, rocky
planets with thin atmospheres close to the
star, a Jupiter - like gas giant just beyond the snowline, and the other giants getting progressively
smaller at greater distances because they move more slowly through their
orbits and take longer to hoover up material.
In August, breathless headlines heralded the discovery of a
small, potentially habitable
planet orbiting Proxima Centauri, a dim red dwarf
star just 4.24 light - years away (SN: 9/17/16, p. 6).
Early in its mission, Kepler managed to find some tantalizing worlds, a handful of supersize cousins of Earth, most of them in clement
orbits around
smaller, cooler, quieter
stars than the sun called M and K dwarfs, but all the setbacks made finding
smaller Earth - sized
planets around sun - like G
stars a very tall order.
That parts - per - million sensitivity should allow Corot to detect the dips in a
star's light caused by a transiting
planet with a radius just twice that of Earth — and perhaps an even
smaller one, provided its
orbit is tighter than Mercury's, so that the
planet completes three transits during the 150 - day viewing period.
They found that one possibly habitable
planet, Kepler - 186f, might
orbit outside its
star's astrosphere, which is
smaller than the one puffed out by our sun.
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
Recently, a newly discovered Earth - sized
planet orbiting Ross 128, a red dwarf
star that is
smaller and cooler than the sun located some 11 light years from Earth, was cited as a water candidate.
The
orbiting probe detects
small dips in the brightness of a
star that occur when a
planet crosses its face.
But astronomers have always wondered about the paucity of close - in brown dwarfs: While many giant
planets have been found in
small orbits, whirling around their sunlike
stars in just a few days, the more massive brown dwarfs appear to shun these intimate relationships.
From this survey data, NASA's James Webb Space Telescope as well as large ground - based observatories will be able to further characterize the targets, making it possible for the first time to study the masses, sizes, densities,
orbits, and atmospheres of a large cohort of
small planets, including a sample of rocky worlds in the habitable zones of their host
stars.
According to a very rough statistical analysis, the new discovery suggests that up to one - third of all red dwarf
stars in the Milky Way galaxy are accompanied by
small, rocky
planets, many of which might be in wider
orbits.
«We have found a
small star, with a giant
planet the size of Jupiter,
orbiting very closely,» said researcher George Zhou from the Research School of Astrophysics and Astronomy at The Australian National University.
And if any
planets similar to these
orbit in their parents
stars» habitable zone, substantially farther from the home
star where liquid water might more likely exist, their atmospheres will lose even
smaller amounts of hydrogen - bearing compounds over time, the researchers note.
The Australian discovery of a strange exoplanet
orbiting a
small cool
star 500 light years away is challenging ideas about how
planets form.
To qualify as potentially life - friendly, a
planet must be relatively
small (and therefore rocky) and
orbit in the «habitable zone» of its
star, which is loosely defined as a location where water can exist in liquid form on a world's surface.
Prabal and his team modelled cases where the
planets are in
orbit close to
small red dwarf
stars, much fainter than our Sun, but by far the most common type of
star in the Galaxy.
The
planet, known as Exo - 7b, lies about 390 light years away and
orbits a
star slightly
smaller and cooler than the Sun.
However, Tuomi's team warns that disturbances on the
star itself, rather than
orbiting planets, may be producing the
small velocity changes in Tau Ceti.
The simulations show that gravitational interactions involving giants in outer
orbits can eject
smaller planets from the system, nudge them into their
stars or send them crashing into each other.
The
smaller team makes the case for at least one, and possibly three,
planets orbiting the sunlike
star HD 1461, some 76 light - years distant.
«We focused on red - dwarf
stars, which are
smaller and fainter than our Sun, since we expect any biomarker signals from
planets orbiting such
stars to be easier to detect.»
Without that detail, astronomers can't tell whether a
star's back - and - forth motions come from a huge
planet moving in a nearly face - on
orbit from our viewpoint, like the minute hand on a clock, or from a
smaller planet in an edge - on
orbit.
As the
planet orbits around its
star, we expect to see regular
small dips in the light coming from the
star as the
planet moves in front of it.
Astronomers using the TRAPPIST - South telescope at ESO's La Silla Observatory, the Very Large Telescope (VLT) at Paranal and the NASA Spitzer Space Telescope, as well as other telescopes around the world [1], have now confirmed the existence of at least seven
small planets orbiting the cool red dwarf
star TRAPPIST - 1 [2].
Based on humankind's admittedly limited experience, habitability seems to mean a
small world — a terrestrial
planet rather than a gas giant like Jupiter or Saturn —
orbiting its
star at a comfortable «Goldilocks» distance that allows water to persist in liquid form.
Borucki says it will be a few years yet before Kepler is able to identify a true Earth analogue — a
small planet on a one - Earth - year
orbit around a sunlike
star.
Many of the first
planets JWST will study are
orbiting small, cool M dwarf
stars, whose outbursts might erode
planets» atmospheres (see «Look to the
stars «-RRB-.
Five
small planets have been found
orbiting this
star, four of which are in very short - period
orbits and are very hot.
In recent years,
planet hunters have been able to measure extremely precise velocities as they hunt for the tiny shifts a
small planet, like the one
orbiting Proxima, induces in its
star, tugging it towards and away from us.
Their results indicate a possible
planet approximately the mass of Neptune — the
smallest yet seen around a sunlike
star —
orbiting every 280 years.