Examples of using Orbital distance in English and their translations into Vietnamese
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This orbital distance makes the planets very hot.
It takes only 4.188 days(or 100.5 hours)to orbit at an orbital distance of 0.0488 AU.[1][2].
Its orbital distance is 1.67 AU, slightly further than Mars and its eccentricity is low.
Com via email, referring to the range of orbital distances where liquid water could exist on a world's surface.
Possible planets of the Gliese 581 system,superimposed on a picture of our own solar system to compare orbital distances.
The actual orbital distances and periods of Phobos and Deimos of 1.4 and 3.5 Martian diameters, and 7.6 and 30.3 hours, respectively.
Kepler discovered 135 planets andover 3,500 planet candidates with a wide range of sizes and orbital distances.
The actual orbital distances of Phobos and Deimos are 1.4 and 3.5 Martian diameters, and their respective orbital periods are 7.6 and 30.3 hours.
The Kepler Space Telescope discovered 135 planets andover 3,500 possible planets of different sizes and orbital distances.
The orbital distance contributes to a colder Antarctic winter(and a warmer Antarctic summer) but the first two effects have more impact.
Launched in 2009, Kepler has been detecting planets andplanet candidates with a wide range of sizes and orbital distances.
They circle their sun-like parentstar every 9.8 days at exactly the same orbital distance, one permanently about 60 degrees ahead of the other.
The planet orbits its host star with about 3% of the Sun's luminosity approximately every 36 days[1]and an orbital radius 0.16 times that of Earth(compared to Mercury's orbital distance of 0.38 AU).
The planet orbits with an eccentricity of 0.0094, which means the orbital distance over the course of its revolution varies by only 0.02 AU.[1].
These events were interpreted as transits of a structure with a period of 808± 2 days,corresponding to an orbital distance of about 2 AU.
HD 164922 b orbits its star every 1,155days at a distance of 2.1 AU(compared to Mars's orbital distance from the Sun, which is around 1.5 AU). It receives only 15% of the sunlight as the Earth does from the Sun.
An azimuthal gap in an annulus of dust at a radius of 102 AU would suggest theformation of at least one small body at an orbital distance of nearly 100 AU.
The eccentricity is 0.115,which means it moves between 1.81 and 2.28 AUs in orbital distance around Gamma Cephei A, which would place it from slightly beyond the orbit of Mars, to the inner Asteroid belt in the solar system.
Along the direction of the star's motion within the Milky Way, this extends out to a distance of 30 AU,or roughly the orbital distance of Neptune from the Sun.
The planet's orbital distance of 0.084 AU(assuming mild eccentricity) lies at the inner edge of its star's habitable zone, which extends from approximately 0.073 to 0.190 AU(for comparison, the habitable zone of the Sun is approximated at 0.5 to 3.0 AU for its different energy emission).
The planet is a typical"hot Jupiter",a planet with a mass half that of Jupiter and orbital distance only 1/24th that of Earth from the Sun.
It is currently the most distant known solar system object from the Sun at a distance of 97 astronomical units, although about forty known TNOs(most notably 2000 OO67 and Sedna), while currently closer to the Sun than 2003 UB313,have greater average orbital distances.
The orbit of an Earth-like planet wouldneed to be centered within 0.68 AU[3](around the orbital distance of Venus), which in a Keplerian system means a 240-day orbital period.
In the final portion of the work(Book V), Kepler dealt with planetary motions,especially relationships between orbital velocity and orbital distance from the Sun.
The amount of gas removed from the outermost layers depends on the planet's size,the gases forming the envelope, the orbital distance from the star, and the star's luminosity.
In 1999 a planet HD 75289 b with half the mass of Jupiter was detected by radial velocity method.[1] This planet is a typical hot Jupiter thattakes only about 3.51 days to revolve at an orbital distance of 0.0482 AU.
HD 240237 b orbits its star with nearly 331 times the Sun's luminosity(331 L☉)every 746 days at a distance of 1.9 AU(compared to Mars' orbital distance from the Sun, which is 1.52 AU).
BD+14 4559 b orbits its star with about 25% of the Sun's luminosity every 268days at a distance of 0.77 AU(close to Venus's orbital distance from the Sun, which is 0.72 AU).
Kepler-419c orbits its host star with 270% of the Sun's luminosity(2.7 L☉)about every 67 days at a distance of 0.37 AU(close to the orbital distance of Mercury from the Sun, which is 0.38 AU).
PSR B1257+12 C orbits its host star with 520% of the Sun's luminosity(5.2 L☉)about every 98 days at a distance of 0.46 AU(close to the orbital distance of Mercury from the Sun, which is 0.38 AU).