<\/p>\n
+ Sometimes, though, enough gravitational<\/strong> force is involved that the two companions speed away from each other at great speeds, resulting in what is known as “runaway” stars.\n<\/p>\n <\/p>\n + It is the center of mass acting in a gravitational<\/strong> field.\n<\/p>\n <\/p>\n + Except for their gravitational<\/strong> pull on one another, they have no effect on each other.\n<\/p>\n <\/p>\n + Moons massive enough for their surfaces to have gravitational<\/strong> collapsecollapsed into a spheroid are highlighted in bold, while the irregular moons are listed in red, orange and gray background.\n<\/p>\n <\/p>\n + These are points of gravitational<\/strong> stability.\n<\/p>\n + They differ in their gravitational<\/strong> effects.\n<\/p>\n <\/p>\n + It is a dimensionless number, the ratio of gravitational<\/strong> forces to viscous forces.\n<\/p>\n <\/p>\n + Instead, it is bent along the gravitational<\/strong> field of a galaxy in front of it.\n<\/p>\n <\/p>\n + Barish “for decisive contributions to the Gravitational<\/strong>-wave observatoryLIGO detector and the observation of gravitational<\/strong> waves”.\n<\/p>\n <\/p>\n + Sources of detectable gravitational<\/strong> waves include binary star systems composed of white dwarfs, neutron stars, or black holes.\n<\/p>\n <\/p>\n + Albert Einstein predicted the possibility of gravitational<\/strong> lensing.\n<\/p>\n <\/p>\n + A stellar black hole is a type of black hole formed by the gravitational<\/strong> collapse of a star.\n<\/p>\n <\/p>\n + In contrast, the more massive globular clusters of stars exert a stronger gravitational<\/strong> attraction on their members.\n<\/p>\n <\/p>\n + They are loosely bound together by mutual gravitational<\/strong> attraction, but they get disrupted by close encounters with other clusters and clouds of gas.\n<\/p>\n <\/p>\n + As the distance is doubled, the gravitational<\/strong> acceleration decreases by a factor of 4.\n<\/p>\n <\/p>\n + Case #2: the observers may be in positions with different gravitational<\/strong> masses.\n<\/p>\n <\/p>\n + The energy emitted by a quasar is gravitational<\/strong> energy, created from mass falling onto the accretion disc around the black hole.\n<\/p>\n <\/p>\n + Einstein\u2019s theory of general relativity predicts that two neutron stars would emit gravitational<\/strong> waves as they orbit a common center of mass, which would carry away orbital energy, and cause the two stars to draw closer together.\n<\/p>\n <\/p>\n + On every plane of creation, energy manifests itself in all forms of matter, thermal energy, potential energy, gravitational<\/strong> energy etc.\n<\/p>\n <\/p>\n + Although the cause is currently unknown but some scientists think that it may be because of the gravitational<\/strong> contact with small moons that orbit near them.\n<\/p>\n <\/p>\n + General relativity predicts that the path of light is bent in a gravitational<\/strong> field; light passing a massive body is deflected towards that body.\n<\/p>\n <\/p>\n + These advances allowed astronomers to detect exoplanets indirectly by measuring their gravitational<\/strong> influence on the motion of their parent stars.\n<\/p>\n <\/p>\n + Total potential energy being the sum of all potential energies — those from gravitational<\/strong> fields, electric fields, and magnetic fields.\n<\/p>\n <\/p>\n + This is because the gravitational<\/strong> field changes across the middle of a body.\n<\/p>\n <\/p>\n + Scientists believe this is caused by the gravitational<\/strong> force of some of Saturn’s moons.\n<\/p>\n <\/p>\n + The centrifugal force of the planets going round the Sun balances the gravitational<\/strong> pull of the Sun.\n<\/p>\n <\/p>\n + Another way gravitational<\/strong> potential energy helps us is by keeping earth and the other planets in orbit in our solar system around the Sun.\n<\/p>\n <\/p>\n + The ossified tendons strengthened the vertebral column against gravitational<\/strong> stress.\n<\/p>\n <\/p>\n + The energy used up when moving up the hill is changed into gravitational<\/strong> potential energy.\n<\/p>\n <\/p>\n + That effect is called gravitational<\/strong> lensing.\n<\/p>\n <\/p>\n + It is believed that Bennu broke off from another asteroid in the asteroid belt, but the gravitational<\/strong> pull of Saturn dislodged it into the range of Earth.\n<\/p>\n <\/p>\n + Best known for his solution to EinsteinEinstein’s equations of general relativity, which describes a the gravitational<\/strong> field outside a non-rotating black hole with no magnetic field.\n<\/p>\n <\/p>\n + In this case, the operator gives a constant multiple of the mass density\u2014when it is applied to a given gravitational<\/strong> potential.\n<\/p>\n <\/p>\n + For example, one can model a gravitational<\/strong> field by a vector field where a vector indicates the acceleration a mass would experience at each point in space.\n<\/p>\n <\/p>\n + As the gas collapses, the central clump grows stronger and the gas heats to extreme temperatures by converting gravitational<\/strong> potential energy to thermal energy.\n<\/p>\n <\/p>\n + As the material moves in, gravitational<\/strong> energy released in that process is transformed into heat and rotational movement.\n<\/p>\n <\/p>\n + G is the gravitational<\/strong> constant.\n<\/p>\n <\/p>\n + Most were once spiral or elliptical galaxies but were deformed by gravitational<\/strong> pull.\n<\/p>\n <\/p>\n + The weight of an object is the measure of the intensity of the force imposed on this object by the local gravitational<\/strong> field.\n<\/p>\n <\/p>\n + In a pond water has gravitational<\/strong> potential energy because of how high it is above sea level.\n<\/p>\n <\/p>\n + It is caused by the changing gravitational<\/strong> forces of bodies which go round each other.\n<\/p>\n <\/p>\n + Their name refers to the long tails produced by tidal action, which is the relative difference between gravitational<\/strong> pulls on the near and far parts of each galaxy.\n<\/p>\n <\/p>\n + Some famous ones are the speed of light, Planck’s constant, the gravitational<\/strong> constant, and Avogadro’s number.\n<\/p>\n <\/p>\n + Also, the strength of any gravitational<\/strong> field slows the passage of time for an object “as seen by an observer outside the field”.\n<\/p>\n <\/p>\n + This is because every particle has positive energy, but it also has gravity, which balances it out with negative gravitational<\/strong> energy.\n<\/p>\n <\/p>\n + In theory, gravitational<\/strong><\/strong> waves transport energy as gravitational<\/strong><\/strong> radiation.\n<\/p>\n <\/p>\n + He wrote a paper on gravitational<\/strong> redshift published in “Nature” in Feb 2010 Nature 18-Feb-2010.\n<\/p>\n <\/p>\n + The NSF has funded improvements for LIGO to increase sensitivity, which allowed them to make the first detection of gravitational<\/strong> waves.\n<\/p>\n <\/p>\n + The formation of black holes may be a major source of gravitational<\/strong><\/strong> waves, so the search for proof of gravitational<\/strong><\/strong> waves has become an important scientific pursuit.\n<\/p>\n <\/p>\n + In the case where the two bodies have the same gravitational<\/strong> force, and that the bodies all have the same mass can be solved exactly.\n<\/p>\n <\/p>\n + When the object comes back down again, the gravitational<\/strong> potential energy is turned back into kinetic energy.\n<\/p>\n <\/p>\n + Because no one has been able to detect gravitational<\/strong> waves directly, the impact of Gravitational<\/strong> Wave Astronomy has been very limited.\n<\/p>\n <\/p>\n + An ideal chain hanging between two supports and acted on by a uniform gravitational<\/strong> force makes the shape of a catenary.\n<\/p>\n <\/p>\n + He showed that the gravitational<\/strong> potential energy lost by the weight in descending was approximately equal to the thermal energy gained by the water by friction with the paddle.\n<\/p>\n <\/p>\n + Measurement of the solar gravitational<\/strong> deflection of radio waves using geodetic very-long-baseline interferometry data, 1979\u20131999.\n<\/p>\n <\/p>\n + These stars are probably in the process of escaping from its gravitational<\/strong> influence.\n<\/p>\n <\/p>\n + Binary pulsar timing has indirectly confirmed the existence of gravitational<\/strong> radiation and verified Albert EinsteinEinstein’s general theory of relativity.\n<\/p>\n <\/p>\n + However, the detection of gravitational<\/strong> waves proves the last prediction of Einstein\u2019s general theory of relativity.\n<\/p>\n <\/p>\n + The speed of the Earth’s movement creates a centrifugal force which balances the gravitational<\/strong> force between the Sun and the Earth.\n<\/p>\n <\/p>\n + The Underground line has hump-backed stations which allow trains to store gravitational<\/strong> potential energy as they arrive and to then use this energy as they leave the stations.\n<\/p>\n <\/p>\n + A gravitational<\/strong> singularity is a term used to describe the center of a black hole where gravity is thought to approach infinity.\n<\/p>\n <\/p>\n![\"gravitational](\"https:\/\/englishteststore.net\/blog\/wp-content\/uploads\/2021\/09\/gravitational-how-to-use.jpg\" "\\"gravitational")
Example sentences of “gravitational”:<\/h2>\n
+ They differ in their gravitational<\/strong> effects.\r\n
+ It is a dimensionless number, the ratio of gravitational<\/strong> forces to viscous forces.\r\n
<\/pre>\nMore in-sentence examples of “gravitational”:<\/h2>\n