Приклади вживання Red dwarf stars Англійська мовою та їх переклад на Українською
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These stars are called red dwarf stars.
Red dwarf stars are the smallest, coolest, and most common type of star. .
Other scientists disagree that red dwarf stars could sustain life.
About 3/4 of all stars in our Galaxy are puny little red dwarf stars.
Because red dwarf stars are so small, the habitable zone is very close to the star. .
It circles a close pair of orange and red dwarf stars every 66 days.
Many red dwarf stars have planets, but let's hope that this one doesn't.
Although low-mass and long-lived, red dwarf stars pose unique threats.
Most of the“earthlike” planets that show up in the news are orbiting very dim red dwarf stars.
Although low-mass, red dwarf stars live for a long time, they also pose unique threats.
But many candidate Earth-sized worlds are in orbit around red dwarf stars, much smaller and cooler than our own.
This is a known problem with red dwarf stars that's led some to question whether they're suitable environments for life to develop.
The problem is that many candidate Earth-sized worlds are in orbit around red dwarf stars, much smaller and cooler than our own.
Despite their dimness, red dwarf stars are good places to look for Earth-like planets.
These stars live much longer than sun-like stars, and have safer habitable zones- where liquid water can exist-than those of lighter red dwarf stars.
The HARPS teamsurveyed a carefully chosen sample of 102 red dwarf stars in the southern skies over a six-year period.
The study found that red dwarf stars might not emit enough ultraviolet(UV) light to kick-start the biological processes most familiar to our planet.
Many newly discovered Earth-size worlds, including ones around TRAPPIST-1 and Proxima Centauri,orbit red dwarf stars whose powerful flares could strip away a planet's atmosphere.
It is one of 15 new exoplanets around red dwarf stars discovered by Japanese astronomer Teruyuki Hirano of the Tokyo Institute of Technology and his team.
Not only could this discovery help us to understand the atmospheres of habitable zone exoplanets in general, butthose of habitable zone rocky exoplanets in close orbit around red dwarf stars.
Researchers have discovered that four old red dwarf stars with masses less than half that of the Sun are emitting X-rays at a much lower rate than expected.
To determine which possibility is correct-- our premature existence or the hazard of low-mass stars--Loeb recommends studying nearby red dwarf stars and their planets for signs of habitability.
The results confirm that red dwarf stars, which weigh between 10 and 50% as much as the sun, are far more prone to unleashing powerful flares that can deliver deadly radiation to nearby planets.
One of the primary outcomes of thenew research highlighted that the planets surrounding red dwarf stars may have exceptionally similar characteristics to planets orbiting solar system stars. .
Given how many red dwarf stars there are in close proximity to the Sun, it means there could be perhaps 100 super-Earth planets in the habitable zones of stars that are less than about 30 light-years distant.
Future telescopes on Earth and in space should helpuncover more Super Earths orbiting red dwarf stars-- believed to be the most common planets and stars in our Milky Way galaxy.
As there are many red dwarf stars close to the Sun the new estimate means that there are probably about 100 super-Earth planets in the habitable zones around stars in the neighbourhood of the Sun at distances less than about 30 light-years.
One major problem with planets orbiting red dwarf stars is that they tend to become tidally locked, with one side of the planet blasted by eternal sunlight while the far side of the planet freezes solid.