Приклади вживання Stars may Англійська мовою та їх переклад на Українською
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Some stars may once have been heavier than they are today.
Ripple patterns in the dust around young stars may show off where giant planets are lurking.
These stars may even have planets, possibly with intelligent life on them.
Arney's research also includes discussion of which of the nearby K stars may be the best targets for future observations.
These stars may even have planets, It's possible, with a reasonable life on them.
The researchers think that a similar gravitational mechanism that produces runaway stars may be also slingshotting these ellipticals.
In some cases, stars may cross the instability strip for a fourth and fifth time when helium shell burning starts.
The presence of such thick dust clouds in the inner regions around some stars may pose an obstacle to the direct imaging of Earth-like planets in the future.
In rare cases, stars may die and come back to life like nothing happened, something that baffles us as well as the scientists.
The presence of such large amounts of dust in the inner regions around some stars may pose an obstacle to the direct imaging of Earth-like planets in the future.
Astronomers believe that these stars may be created after the mid-sized stars(about 1.44 times smaller than our Sun) runs out of fuel to maintain the thermonuclear reaction, and they move in collapserow stage of its life cycle.
But according to a new study by an international teamof astronomers, it appears that these stars may have originated within the Milky Way but were then kicked out.
Scientists believe that some of these compact stars may not be perfectly spherical, and if so, they should emit characteristic gravitational waves, which LIGO and GEO 600 may begin to detect in coming months.
But when Australian stellar theory expert Simon Campbell of the Monash University Centre for Astrophysics, Melbourne,scoured old papers he found tantalising suggestions that some stars may somehow not follow the rules and might skip the AGB phase entirely.
Researchers say that these four strange stars may represent a new type of fate for white dwarfs, who are running out of fuel.
Boson stars may have formed through gravitational collapse during the primordial stages of the Big Bang.[12] At least in theory, a supermassive boson star could exist at the core of a galaxy, which might explain many of the observed properties of active galactic cores.[13].
Researchers say that these four strange stars may represent a new type of fate for white dwarfs, who are running out of fuel.
Objects such as galaxies and nebulae can also absorb, re-emit, or modify light generated within or behind them,and compact stars or exotic stars may contain material which is dark and radio-silent, and as a result we have little evidence of their presence other than through their gravitational interactions.
Such a star would have to be atleast 1,000 solar masses(2.0×1033 kg).[1] These stars may have also been formed by dark matter halos drawing in enormous amounts of gas via gravity, in the early universe, which can produce supermassive stars with tens of thousands of solar masses.[2][3] Stars this large could only form early in the history of the Universe before the hydrogen and helium were contaminated by heavier elements; thus, they may have been very massive Population III stars. .
This supports the theory that double central stars may explain the odd shapes of some of these nebulae, but an even more interesting result was to come.
Although one cannot rule out the possibility that planets around other stars may be confirmed at some future point, it is at least extremely improbable that any of them would fulfil all the requirements needed for life.
Since the 1970s,astronomers have speculated that much of the extra lithium found in young stars may have come from novae- stellar explosions that expel material into the space between the stars, where it contributes to the material that builds the next stellar generation.
The star may thus end up as a black hole.
Besides, the distance between the two double star may change over time.
These differences in the rate of rotation within a star may have a significant role in the generation of a stellar magnetic field.[1].
The star may have planets in orbit as well, but they cannot be detected with current technology.
A star may lose 50 to 70% of its mass during the AGB phase.[7].
Viewed through dust, a star appears fainter and redder than it ordinarily would,and if there is enough dust, the star may not be visible at all.