In August 2006, Pluto was demoted from a planet to
a dwarf planet by the International Astronomical Union (IAU).
Not exact matches
Early images taken
by New Horizons of the
dwarf planet's surface mean we have to rethink how the
planet was formed
The first and second
planets from the
dwarf star are probably less than 15 percent water
by mass, still far wetter than Earth, the researchers found.
Cuk says one possible alternative is that a
dwarf planet or single large asteroid «hundreds or maybe 1000 kilometres across» did the damage after being ripped apart
by gravity when it came too close to Earth or another inner
planet.
Most of the extrasolar
planets that have been found
by telescopes have been located in disks similar to the one around this unusual red
dwarf.
An oversized free - floating
planet formed
by agglomeration would not have a disk, explains Lada, so these
dwarfs must have formed like stars.
RR245 is the largest discovery and the only
dwarf planet found
by OSSOS, which has discovered more than five hundred new trans - Neptunian objects.
Soar over Pluto's seas, mountains, craters and volcanoes of ice in this montage of images released
by NASA from the New Horizons encounter with the
dwarf planet.
But a model of Ceres presented at the LPSC has added a wrinkle
by suggesting comet - like behaviour is only possible at the poles of the
dwarf planet, not the lower - latitude areas where the bright spot has been seen.
This image was taken
by NASA's Dawn spacecraft of
dwarf planet Ceres on Feb. 19 from a distance of nearly 29,000 miles (46,000 kilometers).
Images taken
by NASA's Dawn spacecraft show that a mysterious bright spot on
dwarf planet Ceres could be a plume of water spurting from a deep, icy crater
Even though density measurements suggest that Ceres is roughly one third water
by weight, water ice should rapidly sublimate away into space on the
dwarf planet's airless, sun - soaked surface, so its absence at first would seem to be no surprise.
Other papers in the package also touch on the presence of water ice on Ceres, which had already been reported
by the Dawn team and
by astronomers observing the
dwarf planet from afar.
Red
dwarf stars, which are
by far the most common stars in our galaxy, were once considered unlikely places to find Earth - like
planets, but new studies contradict that view.
[1] The team used data from the UVES spectrograph on ESO's Very Large Telescope in Chile (to determine the properties of the star accurately), the Carnegie
Planet Finder Spectrograph (PFS) at the 6.5 - metre Magellan II Telescope at the Las Campanas Observatory in Chile, the HIRES spectrograph mounted on the Keck 10 - metre telescope on Mauna Kea, Hawaii as well as extensive previous data from HARPS (the High Accuracy Radial velocity
Planet Searcher) at ESO's 3.6 - metre telescope in Chile (gathered through the M
dwarf programme led
by X. Bonfils and M. Mayor 2003 - 2010.
The surface of M -
dwarf planet is illuminated
by visible light.
By throwing a wrench into the theories of
planet and star formation, brown
dwarfs may help fix them
The
planet, dubbed Gliese 581 g, was found to orbit a dim, red
dwarf star every 37 days, according to an analysis
by Steven Vogt of the University of California, Santa Cruz, Paul Butler of the Carnegie Institution of Washington in DC, and their colleagues.
Ever since NASA's New Horizons spacecraft flew
by Pluto last year, evidence has been mounting that the
dwarf planet may have a liquid ocean beneath its icy shell.
One amendment would have left its status open to debate
by creating two categories of
planets — the eight «classical
planets» as well as «
dwarf planets» — that might have seemed to be on equal footing.
SS: TESS will do an all - sky survey to find rocky worlds around the bright, closest M - stars [red
dwarfs that are common and smaller than the sun — and therefore more likely to reveal the shadows cast
by planets], about 500,000 stars.
The globular cluster M4 (left) hosts a pulsar circled
by a white
dwarf (arrow, right) and a Jupiter - sized
planet orbiting both stars.
The observations revealed a slightly elliptical profile for the
dwarf planet, measuring 1610
by 1444 kilometers.
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.
I was rather concerned
by speculation that white
dwarf stars could harbour habitable
planets simply because these stars emit light...
As the
dwarf planet's shadow passed across eight telescopes at five sites in central South America, it blocked light for intervals ranging from 59 seconds to 66 seconds, suggesting that Makemake is a 1500 -
by -1430-km ellipsoid, researchers report online today in Nature.
How such a dense
planet formed is unclear, the researchers say, but it's probably the crystalline vestige of a white
dwarf star whose atmosphere was stripped away
by the parent pulsar.
Red
dwarfs,
by far the most abundant type of star in the galaxy, can create
planet - like signals during their powerful flares.
For the
dwarf planet Pluto, however, the predicted temperature based on the composition of its atmosphere was much higher than actual measurements taken
by NASA's New Horizons spacecraft in 2015.
New Horizons» flyby of the
dwarf planet and its five known moons is providing an up - close introduction to the solar system's Kuiper Belt, an outer region populated
by icy objects ranging in size from boulders to
dwarf planets.
Three new
planets classified as habitable - zone super-Earths are amongst eight new
planets discovered orbiting nearby red
dwarf stars
by an international team of astronomers from the UK and Chile.
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.
Therapist
by day and amateur astronomer
by night, Castro joined the NASA - funded Backyard Worlds:
Planet 9 citizen science project when it began in February — not knowing she would become one of four volunteers to help identify the project's first brown
dwarf, formally known as WISEA J110125.95 +540052.8.
This animation of the
dwarf planet Ceres was made
by combining images taken
by the Dawn spacecraft on January 25, 2015.
Similarly - aged stars moving through space together in a group — described
by astronomers as an association — are of great interest to researchers, because they are considered a prime target to hunt for brown
dwarfs and free - floating
planet - like objects.
GJ 1214 b was discovered
by the MEarth Project, a campaign using eight amateur - size telescopes to monitor nearby M
dwarfs for periodic dimming caused
by transiting
planets.
«Brown
dwarfs are far easier to study than
planets, because they aren't overwhelmed
by the brightness of a host star,» Faherty explained.
New work led
by Carnegie's Jacqueline Faherty surveyed various properties of 152 suspected young brown
dwarfs in order to categorize their diversity and found that atmospheric properties may be behind much of their differences, a discovery that may apply to
planets outside the solar system as well.
After the initial discovery of brown
dwarfs in 1995, scientists quickly realised that they are a natural
by - product of processes that primarily lead to the formation of stars and
planets.
If a large
planet is torn apart
by a
dwarf star, many objects like «Oumuamua could be created at once, says Cuk.
Ehrenreich and his team think that such a huge cloud of gas can exist around this
planet because the cloud is not rapidly heated and swept away
by the radiation pressure from the relatively cool red
dwarf star.
In August 2006 the International Astronomical Union officially demoted Pluto, putting it into the new category of «
dwarf planet,» a sun - orbiting object big enough to be forced into a spherical shape
by gravity but not big enough to clear its own orbit.
Ceres id the first
dwarf planet to be visited
by a spacecraft from Earth.
The New Horizons spacecraft has arrived at Pluto after a decade - long journey, collecting images and data as it flies
by the
dwarf planet at 28,000 mph (45,000 km / h).
These views of
dwarf planet Ceres were taken on 19 February from a distance of about 46,000 kilometres (29,000 miles)
by NASA's Dawn spacecraft.
The highly elliptical orbit, however, suggested that the gravity of an unseen object farther away from the star was pulling the
planet outward, which was later detected
by direct imaging as a methane brown
dwarf — more below.
The mass loading required in this model can be achieved through interaction with the interstellar medium (ISM), the sputtering of the
dwarf atmosphere
by auroral currents, a volcanically active orbiting
planet or magnetic reconnection in the photosphere.
The scientists report that a minor
planet in the planetary system was orbiting around the white
dwarf, and its trajectory was somehow altered, perhaps
by the gravitational pull of a
planet in the same system.
Ceres is the first
dwarf planet to be visited
by a spacecraft (Dawn arrived at Ceres on March 6, 2015, well before New Horizons reached Pluto on July 14).
What's more, it is almost certain that the brown
dwarf population contains a large number of ejected giant
planets — bona fide exoplanets that were booted from their natal systems
by more massive siblings.