Not exact matches
«During the past few years our group,» says David Jones, an astrophysicist at the IAC and another of the authors on the paper, «has discovered that the
planetary nebulae with the biggest discrepancies in their abundances are usually associated with binary central stars which have been through a phase with a common envelope, that is to say the process of expansion of the more massive of the two stars has meant that the
other star is
orbiting within its outer atmosphere, and the viscosity has brought the stars very close to one another.
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.
A bet the former had with
other scientists on the nature of
planetary orbits.
Other theories involve
planetary collisions that knock worlds off course or simply a large mass of materiallike an asteroid that jumps aboard and, by its mass and impact, tilts the once - flat
orbit.
For decades, astronomers have suspected that
planetary nebulae — dazzlingly colorful shrouds of gas cast off by dying stars — owe their weird but often symmetrical shapes to the sculpting magnetic forces of two stars
orbiting each
other at the nebula's center.
Life on planets
orbiting other stars doesn't have to literally broadcast its existence: Radio signals are just one way earthbound scientists might detect biological activity elsewhere in the universe, says Hanno Rein, a
planetary scientist at the University of Toronto, Scarborough, in Canada.
Its dense iron core takes up 42 per cent of its volume, its
orbit is less circular than that of the
other planets, and current
planetary formation models predict Mercury should be closer to the sun and bigger, so we know we're missing something.
Since the late 1980s, scientists have discovered nearly 5,000
planetary bodies
orbiting stars
other than the sun.
But the new evidence comes from a pair of respected
planetary scientists, Konstantin Batygin and Mike Brown of the California Institute of Technology (Caltech) in Pasadena, who prepared for the inevitable skepticism with detailed analyses of the
orbits of
other distant objects and months of computer simulations.
Researchers used software to simulate the
planetary motions within a two - planet system: one being a Jupiter - sized planet (depicted in the artist's concept above)
orbiting its parent star at about the same distance Earth
orbits the sun, and the
other a large planet in a highly tilted
orbit that was slightly larger.
The new study suggests that the «hot Jupiter» WASP - 18b, a massive planet that
orbits very close to its host star, has an unusual composition, and the formation of this world might have been quite different from that of Jupiter as well as gas giants in
other planetary systems.
For this study the researchers used images taken from Earth between 2008 and 2014; they used, among
others, the astronomical cameras PlanetCam (developed by the
Planetary Sciences Group itself) and Astralux, fitted to the telescopes of the Calar Alto Observatory in Almería (Spain); in addition, they used the very high resolution images obtained by t he Cassini spacecraft, which has been
orbiting Saturn since 2004.
Other astronomers find the detections convincing, although most reserve the name «planet» for bodies that form within a
planetary system and
orbit stars, says theorist Alan Boss of the Carnegie Institution of Washington in Washington, D.C. «They should call them «
planetary - mass brown dwarfs,»» Boss says.
In
other cases, when a solar system contains more than 3 massive Jupiter - like planets, the
orbits become unstable by the gravity of these planets and some of them may spin out the
planetary system.
Possibilities for the cause of the orbital disturbance include interactions occurring from the inward migration of planets, the ejection of
other planets from Star A's system through planet - to - planet scattering, or disruption from Star B. (See a larger, interactive animation of the
planetary and potentially habitable zone
orbits of this system, with a table of basic orbital and physical characteristics.)
Starting from the Earth's orbital speed of 30 kilometers per second (km / s), the change in velocity (delta - v) the spacecraft must make to enter into a Hohmann transfer
orbit that passes near Mercury is large compared to
other planetary missions.
In
other words,
planetary orbits that line up with the astrospheric current sheet, which is generally aligned with the star's equator, have a higher probability of being hit by a CME than planets in higher - inclination
orbits.
However, many
others argue that only planemos that directly
orbit stars should qualify as planets, preferring to use the terms «
planetary body,» «
planetary mass object» or «planemo» for similar free - floating objects (as well as planet - size moons).
Some of them are
orbiting extremely close to their parent star like the 51 Peg
planetary system, while
others are found to be at distances comparable to where Mars and Jupiter lie in our solar system.
On the
other hand, the discovery of a brown dwarf companion in a wide
orbit that could perturb dormant comets in an Oort Cloud around Epsilon Indi inwards towards the star's inner
planetary regions may periodically shower an Earth - type, inner planet with catastrophic impacts.
A flotilla of spacecraft
orbiting Mars will be turning their instruments in two directions — one towards Comet Siding Spring, and the
other towards Mars itself, to find out what happens when a
planetary atmosphere brushes against the fuzzy atmosphere of a comet.
And, «In April 2008, it was announced that two simulations of long - term
planetary movement, one at the Paris Observatory and the
other at the University of California, Santa Cruz, indicate a 1 % chance that Mercury's
orbit could be made unstable by Jupiter's gravitational pull sometime during the lifespan of the Sun.
NASA's
Planetary Defense Coordination Office is charged with monitoring the paths of asteroids and
other objects with
orbits that could send them on a crash course with Earth, and planning for response to an actual impact threat.
MAUNAKEA, Hawaii — The search for planets
orbiting other stars in our galaxy has revealed an extraordinary family of planets whose
orbits are so carefully timed that they provide long - term stability for their
planetary system.
Extrasolar planet, also called exoplanet, any
planetary body that is outside the solar system and that usually
orbits a star
other than the Sun.
Such a
planetary orbit is likely to be in synchronous rotation with its host star, so that one side is always facing the star with perpetual daylight while the
other side is in perpetual darkness.
This means that without counting bonuses offered by
other cards the most a planet can have is four buildings, thus four dice, which is why it's important to support valuable planets with fleets in
orbit as attacking players must always destroy ships first before embarking on a
planetary assault.
In the description of the DE200
planetary ephemeris, it is pointed out that, contrary to all the
other objects in the computation which use the Solar system barycentre, the
orbit of our own moon is computed relative to the Earth - Moon barycentre, because then, the
orbit integration will behave nicer numerically — which is good, as the Moon is an object of special interest.
The 9.1 year cycle appears to be linked to a Soli / Lunar tidal cycles, as I also show in the paper, while the
other three cycles appear to be solar /
planetary cycles ultimately related to the
orbits of Jupiter and Saturn.