Astronomers have long suspected that the young, 12 - million - year - old star hosts a massive planet, since it is surrounded by a dusty disc of debris thought to be created by the collision
of rocky bodies and infalling comets.
In the prevailing theory of planet formation, called core accretion, dust grains stick together to form rocky worlds, and
some of these rocky bodies then grow massive enough to attract surrounding gas, becoming gas giants like Jupiter.
Not exact matches
Some
of my clients innocently entered into the world
of dieting, only to find themselves years and years later, with a continually confusing and
rocky relationship with both food and their
bodies.
These
bodies, along with Pluto, are members
of the Kuiper Belt, a population
of rocky potential comets orbiting beyond Neptune.
These «debris disks» are constantly fed by collisions among
rocky bodies — the larger
of which can survive and grow by continued accretion — because the tiny dust grains quickly fall onto the central star or get blown out
of the planetary system.
An infrared telescope has revealed fresh clouds
of dust from gigantic smashups between
rocky bodies, signs that planet - building and destruction take longer and are more violent than astronomers had assumed.
As the years rolled by the planet was losing the fire
of its youth, but it was also slimming down, shedding a few pesky kilometres from its round,
rocky body.
Astrophysicist Alan Boss
of the Carnegie Institution
of Washington thinks this structural similarity gives a reason to suspect that these planets, too, are
rocky bodies that formed much the way Earth did.
The other suggests they arose in a two - stage process called core accretion, in which bits
of material smashed and fused together to form bigger
rocky, icy
bodies.
Until recently, that rule led scientists to think only in terms
of places just like home: temperate,
rocky planets with
bodies of liquid water on their surfaces.
Researchers report that decreasing water pH — one consequence
of rising levels
of carbon dioxide in the atmosphere — dissolves the stony coral's hard skeleton but does not dislodge the soft -
bodied polyps from their
rocky substrate.
If there's gas around and the
bodies get large enough, perhaps something on the order
of 10 Earth masses or so, then you can start pulling some gas in on top
of your
rocky core and make something that looks like a gas giant planet, like Jupiter.
The seeming abundance
of rocky super-Earths lends support to the core accretion model
of planet formation, in which small
rocky bodies collide and clump together to grow into these objects.
With a diameter
of about 1,215 km, the France - sized moon is one
of largest known objects in the Kuiper Belt, the region
of icy,
rocky bodies beyond Neptune.
Indeed, the present - day theory
of planet formation — the build up
of a
rocky planet's core by the accretion
of many small
bodies — is very different from Jeans's.
The presence
of this rock at a site indicates either that material has pushed up through Earth's crust from the mantle (a silicate
rocky shell between the crust and the core with an average thickness
of 2,886 km and depths ranging from 30 km to almost 3,000 km below the crust) or that a celestial
body (a comet, meteor or meteorite) fell there.
Even though many
of the planets orbit their stars very closely and have high temperatures, which in turn causes their hydrogen - rich atmospheres to expand and a fraction
of the gases to escape the planet over time, it's unlikely that the planets will lose enough
of their atmosphere to become
rocky bodies like Earth, the researchers report online today in the Monthly Notices
of the Royal Astronomical Society.
The
rocky body — the largest yet to get a close flyby — seems to have been just large enough to avoid being reduced to a flying pile
of rubble by eons
of collisions with other asteroids.
Last year, rival European and U.S. teams used sensitive new measurements to discover three hot worlds roughly the size
of Neptune (ScienceNOW, 31 August 2004:), which theorists regarded as plausible
rocky bodies.
Analysis
of 166 stars found almost a quarter — much more than expected — had small,
rocky planets, which should force a change in thinking on the overall frequency
of such
bodies.
At the moment, the team's favored idea is akin to the second solution above: that large
bodies of solid metal slowly dropped from the
rocky mantle and into the core to lower the nucleation barrier.
Recent collisions between comets and
rocky bodies within the star system are thought to have generated the surplus
of dust.
Previous research showed Eureka is rich the mineral olivine, which forms in the mantles
of large
rocky bodies but is rare in asteroids.
That heat led to the separation
of the primordial
body into a
rocky crust, an underlying
rocky mantle, and a central metallic core, hallmarks
of planet Earth and the other
rocky planets.
The find is reminiscent
of the solar system's earliest days, when most large,
rocky bodies sported a magma ocean until they cooled down.
Researchers haven't yet confirmed the idea, but further studies should produce new clues about the composition and behavior
of these tiny
rocky bodies — information that someday could help prevent a catastrophic collision with Earth.
In the past, the decay
of radioactive elements and the leftover heat from Titan's formation might have melted nearly all the
body's ice — so the ocean might have extended all the way down to the
rocky core.
As impact glass is a ubiquitous substrate on
rocky bodies throughout the Solar System and likely common on the early Earth, the preservation
of biological activity in impact glass has significant astrobiological implications for life on early Earth as well as for the search for life on other planets.
Such an intriguing metallic planetary
body has not been studied before by any spacecraft; other asteroids visited have been
of the
rocky variety.
Comets, those icy and
rocky bodies with the spectacular long tails
of gas and dust, are common in our Solar System, with several thousand having been discovered so far.
To get a better sense
of the role
of chondrules in a fledgling solar system, the researchers first simulated collisions between protoplanets —
rocky bodies between the size
of an asteroid and the moon.
This is the first time a white dwarf with nitrogen has been discovered, and one
of only a few known examples
of white dwarfs that have been impacted by a
rocky body that was rich in water ice.
nucleus (in astronomy) The
rocky body of a comet, sometimes carrying a jacket
of ice or frozen gases.
In 2006, with the discovery
of several other
rocky bodies similar in size or larger than Pluto, the IAU decided to re-classify Pluto as a dwarf planet.
A speck
of light spotted in October 2015 is a
rocky world more than 3 times more distant than Pluto — the farthest
body in our solar system ever seen.
Calcium - carbonate is attractive as a mineral constituent
of this planet - like
body as incorporating and entraining carbon in
rocky objects (especially their surfaces) is difficult.
Similarly, the terms Neptunes and hot Neptunes refer to planets less than about 10 percent
of Jupiter's mass, and the term super-Earths refers to those planets that may well be
rocky bodies only a few times as massive as Earth.
If the dust trap is formed in the disk, earth - like
rocky planets, small
bodies such as comets, or cores
of gaseous planets may be formed.
Both objects formed among the
rocky and icy protoplanets beyond the Solar System's «ice line» now located around 2.7 AUs, but the early development
of Jupiter apparently prevented such large protoplanets between the gas giant and planet Mars from agglomerating into even bigger planetary
bodies, by sweeping many into pulverizing collisions as well as slinging them into the Sun or Oort Cloud, or even beyond Sol's gravitational reach altogether.
But what mechanism could have raised the temperatures
of the asteroids to this extent if the
rocky bodies were too small to retain the heat from long - lived radioisotopes?»
Abstract: [Abridged] Debris discs around main - sequence stars indicate the presence
of larger
rocky bodies.
In addition to
rocky asteroids and icier
bodies further out from the Sun, many agglomerated into larger planetesimals that eventually collided to form planets like the Earth, and more than 250 minerals, including olivine and zircon, developed within the planetesimals with the help
of melting, collisional shocks, and reactions with water.
So, now, when your
body sends out the signal, «I need sweet food,» your brain can easily interpret it as «Get me a tub
of rocky road ice cream,» instead
of what your
body is actually looking for, which is the energy, vitamins, and minerals that come from root vegetables.
The climactic scenes take place on the beach itself which is a long thin
rocky strip
of land between two
bodies of water in Dorset.
It is in the neighborhood
of Dwejra bay (2 km), where visitors will come across a unique natural phenomenon, the Inland Sea, a shallow
body of water in the niche
of a
rocky coast connected to the sea through a narrow tunnel.
In each montage the artist's photograph
of a
rocky and savage coastal landscape is partially overlaid and merged with enlarged images
of cells from her own
body.
I am making the point that the surface temperature would be more like 299K if, for example, the emissivity
of the dry
rocky planet without water or vegetation were 0.75 rather than the 1.0000 value used for the black
body temperature.