New Hubble telescope images show
ultraviolet radiation from stars born during the universe's adolescent phase.
The Australian telescope was one of several payloads carried into space by the shuttle Endeavour to observe
ultraviolet radiation from stars and galaxies.
Here, the bright orange lanes have been whittled away by
ultraviolet radiation from the star, turning them into knots with cometlike tails.
This discovery refutes existing theories, indicating that
ultraviolet radiation from the star would destroy molecular gas and dust, and bringing the first direct detection of ionized gas wind along with a supersonic jet and an accretion disk.
Not exact matches
These globules are under fierce bombardment
from the
ultraviolet radiation from nearby hot young
stars.
Larger Bok globules in quieter locations often collapse to form new
stars but the ones in this picture are under fierce bombardment
from the
ultraviolet radiation from nearby hot young
stars.
Scientists think that when the first
stars were born, these luminous objects and the galaxies they formed eventually pumped out X-rays and
ultraviolet radiation that ripped electrons
from their proton partners.
Ultraviolet light
from early, blueish
stars (illustrated) interacted with hydrogen gas, causing it to absorb background
radiation, and creating a signature scientists have now detected.
Although Proxima Centauri's dimness provides the planet with a balmy climate, the
star is prone to outbursts of harsh X-ray and
ultraviolet radiation, which could damage any chance of life on the planet — X-rays hit the surface 400 times more often than those
from the sun pummel Earth.
A computer model developed by the team suggests that the grains must reach the size of boulders within a million years; otherwise, the dust particles and circumstellar gases will be blown apart by fierce
ultraviolet radiation from the nebula's hottest, most massive young
stars.
Using data gleaned
from the Hubble telescope, researchers have calculated the amount of
ultraviolet (UV)
radiation the planets receive
from their
star, a Hubble press release reports.
This
radiation comes
from established
stars, rather than newborn
stars that blaze furiously in
ultraviolet light.
Astronomers have known for about a decade
ultraviolet and X-ray
radiation from the main
star in HD 189733 are evaporating the atmosphere of HD 189733b over time.
A nearby
star features a comet - like tail that could be the outer reaches of a protoplanetary disk evaporating under the intense
ultraviolet radiation from IRS 2.
Gas and dust clouds in 30 Doradus, also known as the Tarantula Nebula, have been sculpted into elongated shapes by powerful winds and
ultraviolet radiation from these hot cluster
stars.
When the
star's
ultraviolet radiation strikes the gases in the nebula, they heat up, giving out
radiation ranging in wavelength
from blue — emitted by hot oxygen in the bubble near the
star — to yellow — emitted by hot hydrogen and nitrogen.
The formation of a stratosphere layer in a planet's atmosphere is attributed to «sunscreen» - like molecules, which absorb
ultraviolet (UV) and visible
radiation coming
from the
star and then release that energy as heat.
Eventually, as the early
stars grew in numbers and brightness, they would have emitted enough
ultraviolet radiation to «reionize» the hydrogen, removing the electrons
from their bonded protons and neutrons.
The first
stars, however, also began emitting intense
ultraviolet radiation that «re-ionized» neutral hydrogen atoms formed after the Big Bang by tearing electrons
from their proton nuclei.