Examples of using Massive objects in English and their translations into German
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Political
Massive objects have two fundamental properties.
Black holes are the most massive objects in the universe.
Less massive objects like our sun remained close to the original nebula.
And if both had black holes at their centers, what would happen to those massive objects?
Massive objects like galaxies bend light rays that travel near them, just as a glass lens does.
Many companies have gone bigger, constructing and installing massive objects in public spaces.
The two are the most massive objects in the asteroid belt and are two of the last major unexplored bodies in the inner Solar System.
The goal behind his ERC Consolidator Grant is todevelop methods for the quantum control of levitated massive objects.
The computation of extensive regions and long or massive objects often involves many elements for discretization in the computational domain.
The upper with a somewhat longer arm, directed upwards,has been created with thoughts of hanging heavier and more massive objects.
Thus two massive objects which are rapidly circling each other should emit gravitational waves which are transmitted at speed c throughout space.
The precisely cast cast guarantees great durability,thanks to what you can successfully place massive objects on the resulting wall shelf.
Usually, under the influence of gravity of more massive objects, it rotates around them in its orbits, for example, like the moon around the Earth.
The presented shelf console is the extraordinary possibility to create a massive and individually designed shelf,which with its reliable execution can absorb massive objects.
What once led to massive objects with a shape strongly constrained by the minimum wall thickness required, can now engender quite different results.
Galaxy clusters have huge mass, and the Theory of General Relativity says massive objects bend light as it passes by them, a phenomenon known as gravitational lensing.
Black holes are massive objects which become so highly collapsed that their gravity attracts anything within proximity, powerful vacuum cleaners of near space.
Taking the path of light and its velocity to be the only reliable constant in the universe, he came to the conclusion thatlight would be bent by the presence of massive objects.
If there were no massive objects these things would go flying off, or at least go at a much slower rate because all that determines how they go around is how much mass is inside its orbit.
Massive objects such as RCS2 J2327 have such a strong influence on their surroundings that they actually warp the space around them- this effect is known as gravitational lensing, and can cause light from more distant objects to be bent, distorted, and amplified, allowing us to see galaxies that would otherwise be far too distant for us to detect.
Sir, we're detecting a massive object emerging from hyperspace.
The closer you are to a massive object, the more the pull of its gravity slows down anything trying to escape from it.
This is similar to what happens to light passing close to a massive object that deforms the space surrounding it.
This titanic mass is similar to that of the largest structures observed in the Universe today,but finding such a massive object in the early Universe surprised astronomers.
There is no new massive object traveling toward Earth, any more than there is a comet traveling across the skies in the path put forth for Hale-Bopp.
It is well known that a very massive object, such as a huge galaxy or a cluster of galaxies, can behave as a kind of lens that bends, amplifies or even replicates the images of fainter and more distant, background objects. .
Within about 5 years, we will be able to distinguish the shadow of the black hole, the dark depression inside the event horizon,the well in the curvature of space-time produced by this massive object, against the background of the bright hot gas surrounding it.
His tree of life is a massive object.
Deflection of light by the Sun===Henry Cavendish in 1784(in an unpublished manuscript) and Johann Georg von Soldner in 1801(publishedin 1804) had pointed out that Newtonian gravity predicts that starlight will bend around a massive object.
Examination of the four quasar spectra confirmed that these were indeed four distinct quasars rather than multiple images of a single quasar; a phenomenon that canoccur through gravitational lensing, when light is bent by the gravity of a massive object in the foreground.