Examples of using Surface gravity in English and their translations into Portuguese
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Equatorial surface gravity m/sec^2.
The combination of the radius andthe mass of a star determines the surface gravity.
Titan's surface gravity is 0.14 g.
Stellar microturbulence varies with the effective temperature and the surface gravity.
The surface gravity on Mars is more than a third of Earth's.
Due to its mass it is likely to have a surface gravity 6-8 times that of Earth.
The surface gravity is also high, over 50 times that of Earth.
Trivia Kerbin has the same equatorial radius as Tylo(600,000m) yet Tylo's surface gravity is much lower than Kerbin.
Their surface gravity is typically between 104 and 106 meters per second squared.
Mass loss is largest for high luminosity stars with low surface gravity and enhanced levels of heavy elements in the photosphere.
Its surface gravity is expected to be about six to eight times that of Jupiter's.
The Sun has just under twice the surface gravity of Kerbin, thus only slightly more than Eve's.
Mars' surface gravity is 38 percent of Earth's, while it rotates around its axis in about the same time as Earth.
The planet has a large mass(nine times the mass of Jupiter), and a surface gravity 25 times that exerted by the Earth.
Low gravity===The surface gravity on Mars is 38% of that on Earth.
A PMS star will have a larger radius than a main-sequence star, andthus be less dense and have lower surface gravity.
This means that their surface gravity and density go up proportionally to their mass.
Using the stellar spectrum,astronomers can also determine the surface temperature, surface gravity, metallicity and rotational velocity of a star.
WASP-13's surface gravity is measured at 4.04 km/s2, while the rate at which it rotates is at most 4.9 km/s.
This indicates its mean density is twice that of Earth and its surface gravity approximately 24 times that on Earth, almost equal to the Sun.
Escape==Surface gravity, the force that holds down an atmosphere, differs significantly among the planets.
For all 150,000 stars that were watched for transits by Kepler, there are estimates of each star's surface temperature,radius, surface gravity and mass.
Values for the surface gravity, log(g), of O class stars are around 3.6 cgs for giants and 3.9 for dwarfs.
In addition, stars may be classified by the luminosity effects found in their spectral lines, which correspond to their spatial size andis determined by the surface gravity.
Gravity(g) modes, driven by buoyancy,*: Surface gravity(f) modes, akin to ocean waves along the stellar surface. .
The surface gravity can influence the appearance of a star's spectrum, with higher gravity causing a broadening of the absorption lines.
Kepler-452b has a probable mass five times that of Earth, and its surface gravity is twice Earth's, though calculations of mass for exoplanets are only rough estimates.
Surface gravity and temperature are also critical to within a few percent for the earth to have a life-sustaining atmosphere- retaining the right mix of gases necessary for life.
These lists can also be sorted according to an object's mass and,for the largest objects, volume, density and surface gravity, insofar as these values are available.
The effective temperature and surface gravity were also obtained by using photometric calibrations and through the trigonometric technique.