Keplerian disks, that is disks with Keplerian rotation, are very likely to eventually form
planets in stable orbits.
Not exact matches
For example, William Paley, already
in 1802,
in his treatise Natural Theology, pointed out that if the law of gravity had not been a so «called «inverse square law» then the earth and the other
planets would not be able to remain
in stable orbits around the sun.
Planets don't form in such tidy arrangements, which suggests that the TRAPPIST - 1 planets were born in orbits farther out, before migrating inward and becoming trapped in the stable, resonant
Planets don't form
in such tidy arrangements, which suggests that the TRAPPIST - 1
planets were born in orbits farther out, before migrating inward and becoming trapped in the stable, resonant
planets were born
in orbits farther out, before migrating inward and becoming trapped
in the
stable, resonant
orbits.
In the old view, the planets formed in an orderly manner, born from a swirling disk of gas and dust, known as the solar nebula, into stable orbits at their present locations from the su
In the old view, the
planets formed
in an orderly manner, born from a swirling disk of gas and dust, known as the solar nebula, into stable orbits at their present locations from the su
in an orderly manner, born from a swirling disk of gas and dust, known as the solar nebula, into
stable orbits at their present locations from the sun.
For decades we have blindly checked the sky overhead or targeted stars that are old enough, metallic enough and
stable enough to have rocky
planets in the right
orbits.
In our universe the laws of physics seem precisely calibrated to allow the existence of long - lived stars,
planets with
stable orbits, and molecules that allow complex chemistry.
The new
planets completely fill up the habitable zone of Gliese 667C, as there are no more
stable orbits in which a
planet could exist at the right distance to it.
They eliminated those with orbital radii less than one tenth that of Earth's, because at that distance moon systems might not remain
in stable orbits around their
planets on billion - year timescales.
He pointed out that there are many close -
orbiting planets around middle - aged stars that are
in stable orbits, but his team doesn't know how quickly this young
planet is going to lose its mass and «whether it will lose too much to survive.»
An Earth - type
planet could have liquid water
in a
stable orbit centered around 0.036 AU from Star B — well within the orbital distance of Mercury
in the Solar System.
If so, then conditions would be more favorable for the existence of
stable orbit for an Earth - like
planet (with liquid water) centered around 1.5 AU from around Iota Persei — around the orbital distance of Mars
in the Solar System.
Recent numerical integrations, however, suggest that
stable planetary
orbits exist: within three AUs (four AUs for retrograde
orbits) of either Alpha Centauri A or B
in the plane of the binary's
orbit; only as far as 0.23 AU for 90 - degree inclined
orbits; and beyond 70 AUs for
planets circling both stars (Weigert and Holman, 1997).
An Earth - type
planet could have liquid water
in a
stable orbit centered around 1.18 AU from Star A — between the orbital distances of Earth and Mars
in the Solar System.
For an Earth - type
planet around HD 189733 A to have liquid water at its surface, it would need a
stable orbit centered around 0.5 AU — between the orbital distances of Mercury and Venus
in the Solar System (with an orbital period around 150 days assuming a stellar mass around 82 percent of Sol's.
If a small, rocky
planet can develop without the interference of
planet b, then
stable orbits appear to be possible
in the inner portion of the habitable zone (Noble et al, 2002,
in pdf; and Jones and Sleep, 2003).
If so, then conditions would be more favorable for the existence of
stable orbit for an Earth - like
planet (with liquid water) centered around 1.15 AU from around 15 Sge — between the orbital distances of Earth and Mars
in the Solar System.
Assuming that the spectroscopic companion B does not preclude a
stable inner planetary
orbit, the distance from Star A where an Earth - type
planet would be «comfortable» with liquid water is centered around only 0.457 AU — between the orbital distances of Mercury and Venus
in the Solar System.
If so, then conditions would be more favorable for the existence of
stable orbit for an Earth - like
planet (with liquid water) centered around 1.12 AU from around 37 Gem — between the orbital distances of Earth and Mars
in the Solar System.
They remain
in stable orbits either leading or following the
planet in its own
orbit, 60 degrees before or after the
planet.
In this area, gravity from the sun and the planet pull equally, keeping the satellite in a stable orbi
In this area, gravity from the sun and the
planet pull equally, keeping the satellite
in a stable orbi
in a
stable orbit.
An Earth - type
planet could have liquid water
in a
stable orbit centered around 3.5 AU (within a predicted habitable zone ranging between 2.3 and 4.8 AUs) from Star A — between the orbital distances of the Main Asteroid Belt and Jupiter
in the Solar System (NASA Stars and Exoplanet Database).
Orbity.io is a tricky and very addictive massively multiplayer browser based rocket game
in which players attempt to maintain
stable orbits around the
planet Earth for as long as possible or take off and explore space.