Pluto has long been a misfit in the prevailing theories of the solar system's origin: it is thousands of times less massive than the four gas -
giant outer planets, and its orbit is very different from the well - separated, nearly circular and co-planar orbits of the eight other major planets.
False color, for the sake of drama, got a lot of reinforcement when
the giant outer planets were photographed during the Voyager mission in the late 1970s and 1980s.
Gladman speculates that
the giant outer planets captured passing chunks of rock or ice while the solar system was forming.
The new data also give scientists clues to a long - standing mystery about the atmospheres of
giant outer planets.
As
those giant outer planets grew, their powerful gravity flung much of that debris outward.
Not exact matches
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.
Six
planets orbit a star roughly the size of the sun, and like our solar system, the
outer planets are gas
giants while the inner ones seem to be denser.
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.
The star Kepler 36 has two
planets: an inner rocky world slightly larger than Earth, and an
outer gas
giant about the size of Neptune.
This lower limit was intriguing because the
outer edge of the hole is about as far from its star as the
giant planets in our solar system are from the sun.
«Ceres or ammonia - rich material from the
outer solar system could have been implanted in the Asteroid Belt as a result of orbital perturbations exerted by the
giant planets» early in the solar system's history, De Sanctis says.
A new analysis of
outer solar system orbits suggests that there really could be a hitherto unseen
giant planet orbiting far from the sun — but what are the implications?
The two gas
giant planets did a gravitational dance with the sun and each other that sent them hurling in then back out to the
outer solar system.
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.
While we have four inner rocky
planets and four
outer gas
giants, many other systems have «hot Jupiters» very close to their star.
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.
By using models of how
planets shape a debris disc, the team found that «eccentric» versions of the
giant planets in the
outer solar system could explain the observed properties of the ring.
Robotic spacecraft, such as Pioneer 10 and 11 and the Voyager probes, gave us our first close - ups of the gas
giant planets in the
outer solar system.
Useful for launching larger interplanetary science payloads such as Asteroid Redirect Mission, Mars Sample Return, Jupiter Europa Orbiter, Saturn / Titan Sample Return, Ice
Giant Exploration,
Outer Planet Sample Return, Large Telescopes and In - Space Infrastructres.
During a presentation at NASA's
Outer Planets Assessment Group in 2013, Hofstadter stressed the significance of mounting a mission to the ice
giants.
This gaseous,
giant,
outer planet has a visible ring system and over 20 moons, the largest of which is Titania.
Called «NASA's Leadership and America's Future in Space,» the report said that studying the
outer gas
giant planets (such as Saturn) help scientists learn about their atmospheres and internal structure.
Neptune has a ring system, just like all the
giant gaseous
outer planets.
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.
«The composition and chemistry of ice
giant atmospheres provides clues about their formation, evolution and current state,» explained a research paper referenced as part of NASA's
Outer Planets Assessment Group Meeting in Laurel, Maryland.
A Neptune - like gas
giant may orbit Vega in an
outer orbit, «pushed out» after its formation by a larger Jupiter - like
planet in an inner orbit (more).
a. Gases dissipate rapidly in the vacuum of
outer space, especially the lightest two gases — hydrogen and helium, which comprise most of the mass of the
giant planets.
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.
On June 16, 2008, a team of astronomers announced at the 2008 Extra Solar Super-Earths Workshop in France their discovery of one «super-Earth» type
planet in a tight orbit around this star with two other gas
giant planets in
outer orbits (ESO press release and Bouchy et al, 2009).
Detecting water on Ceres supports models of the solar system in which
giant planets, such as Jupiter, migrated to their current positions, mixing material from the
outer and inner regions of the solar system.
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.
HDST would also provide detailed data on the interaction of each of the
outer planets with the solar wind and give planetary scientists the ability to search for remote, hidden members of our solar system ranging in size from dwarf
planets to ice
giants like Neptune.
«ALMA Sheds Light on
Planet - Forming Gas Streams — Tantalising signs of flows feeding gas - guzzling giant planets» The above article published in January 2013 by S. Casassus describes the planet formation in the disk closer to the central star, but there is no discussion on the planet formation in the outer
Planet - Forming Gas Streams — Tantalising signs of flows feeding gas - guzzling
giant planets» The above article published in January 2013 by S. Casassus describes the
planet formation in the disk closer to the central star, but there is no discussion on the planet formation in the outer
planet formation in the disk closer to the central star, but there is no discussion on the
planet formation in the outer
planet formation in the
outer disk.
Low - to medium - mass stars, such as the sun, will eventually swell up into red
giants, eventually shedding their
outer layers into a ring known as a planetary nebula (early observers thought the nebulae resembled
planets such as Neptune and Uranus).
These
planets are called gas
giants, because they are mostly made of gas and do not have a solid
outer crust.
That two of the first three
planets were larger than Earth but smaller than the Solar System's four
outer gas
giants was also unexpected.
Although 220 km (137 miles) in diameter, the largest
outer moon, Phoebe, is dark with a retrograde, highly inclined orbit and so may be a captured icy body from the Edgeworth - Kuiper Belt rather than a moon that formed with the
giant planet.
An audacious plan from the start, the goal was to explore a virtually unknown region of the
outer Solar System, including the gas
giant planets Jupiter, Saturn, Uranus, and Neptune, using twin Voyager spacecraft.
When Earth is threatened by
giant machine life from
outer space, the
planet's greatest heroes unite - but will they be enough?
There are very deep reasons for the differences in climate among the terrestrial, or Earth - like,
planets (as opposed to the Jupiter - like gas
giants in the
outer solar system), and I mean that literally.