Dust at the outermost planet's orbit moves too slowly to snowball
into a giant planet, and the star's heat would prevent the innermost disc collapsing, they say (Nature, DOI: 10.1038 / nature09684).
FOND FAREWELL The Cassini spacecraft took this last look at the Saturn system two days before plunging
into the giant planet's atmosphere.
That's when mission planners project radio communications will be lost with the two - ton, bus - size spacecraft as it plunges
into the giant planet's turbulent atmosphere at more than 122,000 kilometers per hour.
Dust at the outermost planet's orbit moves too slowly to snowball
into a giant planet, and the...
At 8:53 P.M. Pacific time, ground controllers received a telemetry tone of 2,327 hertz — equivalent to the highest D note on a piano keyboard — indicating that Juno's 35 - minute engine burn had slowed the spacecraft enough to slip
into the giant planet's gravitational embrace.
As Jupiter accreted
into a giant planet, its gravitational pull began to disturb the orbits of the nearest planetesimals so that collisions became more violent.
Beyond this point rapid gas accretion ensues, turning the core
into a giant planet in a relatively short period of time.
Not exact matches
Ask an astronomer how
planets form, and she'll say parts of a
giant wheel of gas and dust around a newborn star, called a protoplanetary disk, somehow collapse
into blobs.
At any time a
giant asteroid could smash
into our
planet and change our world forever.
Meeting the Neighbors A century ago, our solar system seemed split
into two tidy groups: the terrestrial inner
planets — Mercury, Venus, Earth, Mars — and the
giant, gaseous outer worlds.
Their first instinct was to run simulations involving a
planet in a distant orbit that encircled the orbits of the six Kuiper Belt objects, acting like a
giant lasso to wrangle them
into their alignment.
They were the first human missions to those two
giant planets and then afterwards, they just shot out of the solar system and are now heading
into deep interstellar space.
The findings will influence how ice
giants are studied in future and could help astronomers classify newly discovered
planets as they look deeper
into space.
Red
giant stars may be tricking us
into thinking they have
planets when they don't.
All that changed drastically and violently 64.5 million years ago when a
giant asteroid slammed
into the
planet north of the Yucatà¡ n Peninsula, apparently creating a worldwide pall of dust, ash, and debris.
The gravity of the other
giant planets also tugs on Uranus, so this must be taken
into account.
A
giant asteroid impact in the dwarf
planet's past offers new insights
into the possibility of an ocean beneath its surface.
One lesser known casualty was the Galileo mission to Jupiter, a $ 1 billion NASA spacecraft designed to orbit the
giant planet, study its many moons and drop a probe
into its atmosphere.
The red
giant will eventually cast off its entire carbon - rich envelope, leaving behind only a small, hot core, while its lost material spreads
into space, ready to enrich
planets that have yet to be born with the key element on which all terrestrial life is based.
The work could explain why the
planet has a relatively small heart, and paints a grisly picture of the early solar system, where massive, rocky «super-Earths» were snuffed out before they could grow
into gas
giants.
Incidentally, that's the same fate that awaits Mercury and Venus, the two innermost
planets in our own solar system, when the sun grows
into a bloated red
giant star some 5 billion years from now.
Several teams are racing to spot
Planet Nine, a hypothetical giant planet in the outer reaches of the solar system, based on the way it may have shepherded six objects into clustered o
Planet Nine, a hypothetical
giant planet in the outer reaches of the solar system, based on the way it may have shepherded six objects into clustered o
planet in the outer reaches of the solar system, based on the way it may have shepherded six objects
into clustered orbits.
This finding could offer new insights
into the timeline for
giant planet formation around young stars.
The resonance may date back to the
planets» births and thus may yield insights
into the formation of
giant planets around other stars, including our sun.
Comet Wild - 2 used to orbit beyond the orbit of Jupiter, but it made an unusually close approach to the
giant planet in September 1974 and got catapulted
into the inner solar system.
Theoretical models predict that migration occurs either early in the lives of
giant planets while still embedded within the protoplanetary disk, or else much later, once multiple
planets are formed and interact, flinging some of them
into the immediate vicinity of their star.
Piecing those clues together, the two Alvarezes proposed a radical idea: The mass extinction that wiped out the dinosaurs 65 million years ago was caused by the impact of a
giant asteroid, which unleashed a globe - spanning cloud of debris and plunged the
planet into darkness for months.
She and her team also showed the
giants pull the few remaining inner
planets into more elliptical and inclined orbits — the same kind seen in many of the single systems Kepler has spotted.
The
giants pull the few remaining inner
planets into more elliptical and inclined orbits — the same kind seen in many of the single systems Kepler has spotted (arxiv.org/abs/1609.08110).
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.
But interactions with the newly formed
giant planets ejected many of those comets
into interstellar space, flung others out
into what would become the Oort Cloud, and knocked some
into elongated, somewhat shorter orbits in what is known as the scattered disk.
From the spread of the fragments, astronomers have calculated that the comet passed so close to Jupiter last July that it broke
into at least 17 pieces, which now orbit the
giant planet about once every two years (This Week, 17 April).
Plate tectonics is special to Earth: The
planet's crust is divided
into giant, mobile plates.
Recently detected ripples in the gas
giant's rings carry signatures of the
planet's interior structure, offering new insights
into what lies far beneath Saturn's cloud tops.
This could point to diversity in how and where
giant gassy
planets like this come
into being.
However, in a few billion years our sun will become a red
giant, engulfing Mercury and Venus, turning Earth and Mars
into sizzling rocky
planets, and warming distant worlds like Jupiter, Saturn and Neptune — and their moons — in a newly established red
giant habitable zone.
Scientists have debated for years what will happen to our
planet when the sun's fusion furnace begins to run out of fuel and swell
into a red
giant a few billion years from now.
Maunakea, Hawaii - When NASA's Cassini spacecraft plunges
into the atmosphere of Saturn on Sept. 15, ending its 20 years of exploration, astronomers will observe the
giant planet from Earth, giving context to Cassini's final measurements.
In only a few billion years, our own sun will turn
into a red
giant star, expand and engulf the inner
planets, possibly even Earth.
At the January 2002, 199th Meeting of the American Astronomical Society in Washington, DC, two teams of astronomers announced that the cold dust in Vega's circumstellar disk is at least partly gathered
into large clumps, in a characteristic shape that suggests the gravitational influence of a
giant planet in an eccentric orbit (Abstracts for sessions 66.04 and 66.05, and CfA press release).
As for how it was formed, astronomers are stumped as a
planet of that size would usually turn
into a gas
giant (like Jupiter) in the early stages of formation.
They also hope to study «ring rain,» particles that escape from the gas
giant's rings and flow
into the
planet itself, the website noted.
According to NASA, due to the gravitational pull of the
planet it should have pulled in a massive amount of gas that would eventually increase its size and transform it
into a gas
giant.
At the outer fringes of the system, the gravitational influence of a hypothetical
giant planet (bottom left) captures comets
into a dense, massive swarm (right) where frequent collisions occur.
During this period, the
giant planets within the Solar System migrated in toward the Sun and then out again until they settled
into the orbits they maintain today.
Professor Emma Bunce from the University of Leicester awarded Chapman Medal for outstanding research
into gas
giant planets
Looking farther,
into the outer solar system, Webb's observations will give us a better picture of the seasonal weather and climate on our
giant planets and their moons.
The map provides a tantalizing glimpse of
giant filamentary structures extending across millions of light - years, and paves the way for more extensive studies that will reveal not only the structure of the cosmic web, but also details of its function — the ways that pristine gas is funneled along the web
into galaxies, providing the raw material for the formation of galaxies, stars, and
planets.
The larger gas
giants are massive enough to keep large amounts of the light gases hydrogen and helium close by, although these gases mostly float
into space around the smaller
planets.
Combining all of the measurements across the entire field of view allowed the team a tantalizing glimpse of
giant filamentary structures extending across millions of light - years, and paves the way for more extensive studies that will reveal not only the structure of the cosmic web, but also details of its function — the ways that pristine gas is funneled along the web
into galaxies, providing the raw material for the formation of galaxies, stars, and
planets.