He routinely speaks in a loud, basso voice which Anderson often likens to the sound of a hurricane or avalanche, much as his physical bulk is often compared to a mountain or a Jovian planet.
32.
With a minimum mass just 18 times that of the Earth, the planet is likely a " hot Neptune " planet, a small Jovian planet, or possibly a large terrestrial planet ( a super-Earth ).
33.
A Jovian planet should not have been able to form so close to the primary, and with no disk material beyond 1 AU, a planet should not have been able to form beyond that distance to migrate inward.
34.
:If you mean extraterrestrial life, the general assumption seems to be that it would need an environment similar to that of Earth, which would mean a small, terrestrial planet / asteroid or a moon of a larger, Jovian planet.
35.
The alternative term " jovian planet " refers to the Roman god Jupiter the genitive form of which is " Jovis ", hence " Jovian " and was intended to indicate that all of these planets were similar to Jupiter.
36.
:The good news is, high gravity isn't likely to be a limiting constraint, since only the larger of the Jovian planets, which are inhospitable for a number of other reasons, are likely to have too much gravity for us to stand.
37.
The Keplerian fit of the RV data suggested an orbital solution for a close-in massive planet with an orbital period of 7.7834 days . Moreover, the presence of a close-in massive jovian planet could explain the high level of stellar activity detected.
38.
For example, we could have the terrestrial planets ( Mercury, Venus, Earth, and Mars ), the Jovian planets ( Jupiter, Saturn, Uranus, and Neptune ), the trans-neptunian planets ( Kuiper Belt objects such as Pluto, Nebular110 22 : 22, 20 July 2006 ( UTC)
39.
Recently we are studying on solar system planets moons and Kuiper and asteroid belt, our work shows a bit mass increasing of jovian planets, after acceptance of such calculations I can say it here .-- talk ) 05 : 51, 4 October 2011 ( UTC)
40.
"' Kepler-39b "'( formerly known as "'KOI-423b "'), is a confirmed extrasolar object ( either a Jovian planet or brown dwarf because of its mass ) discovered orbiting the F-type star Kepler-39 . It is eighteen times more massive than Jupiter, and is about five fourths its size.
