This is much closer to
the star than the dust discs of other main - sequence stars with excess far - infrared radiation.
Not exact matches
Infrared radiation passes through interstellar
dust much more easily
than visible light, so by looking at the infrared light from a galaxy we can learn about the new
stars forming within the clouds of
dust and gas.
This is because the
dust in dark nebulae absorbs and scatters blue light from
stars more
than red light, tinting the
stars several shades more crimson
than they would otherwise be.
Now, thanks to a $ 107,000 Kickstarter fund and the work of more
than 200 scientists, researchers know it's not extraterrestrials, but space
dust that's causing the erratic and extreme dips in brightness around Tabby's
star.
The thickest
dust disks are most prominent for the youngest
stars, less
than 100 million years old.
More strangeness: Both Antares
stars are embedded in an odd nebula composed of fine metallic
dust rather
than gas.
Spitzer is conducting a systematic study of the
dust around more
than 300 nearby
stars, each about 2.5 times as massive as the sun.
Watch the changing
dust density and the growth of structure in this simulated debris disk, which extends about 100 times farther from its
star than Earth's orbit around the sun.
For more
than 30 years, astronomers have known that Vega has a massive belt of cold
dust far from the
star, analogous to our solar system's Kuiper Belt.
The HOSTS Survey has determined that the typical level of zodiacal
dust around other
stars — called «exo - zodiacal
dust» — is less
than 15 times the amount found in our own solar system's habitable zone.
New work from a team of Carnegie cosmochemists published by Science Advances reports analyses of carbon - rich
dust grains extracted from meteorites that show that these grains formed in the outflows from one or more type II supernovae more
than two years after the progenitor
stars exploded.
However, at those wavelengths,
stars glow 10,000 times brighter
than the
dust.
Or by nature itself: there is a chance that Alpha Centauri's
stars are surrounded by significantly more light - scattering
dust than our own Sun, which could prevent a small telescope from seeing any planets.
Stars with more
than that amount of
dust make poor targets for future exoplanet imaging missions, as planets would be difficult to see through the haze.
Rather, they analyzed microscopic silicon carbide, SiC,
dust grains that formed in supernovae more
than 4.6 billion years ago and were trapped in meteorites as our Solar System formed from the ashes of the galaxy's previous generations of
stars.
She says that the uncertain science of measuring
dust around
stars means that there may have been more present at TYC 8241 2652
than Song believes.
The discovery offers an added benefit: astronomers will be able to study the evolution of the
stars much more easily
than if they had been cloaked inside their parent galaxy's clouds of
dust.
By examining infrared data taken earlier by the Spitzer Space Telescope, they discovered a swath of
dust particles ranging in size from 0.1 to 20 microns (finer
than a split hair) that added up to the mass of a large asteroid and, based on their warmth, were strewn about 1.8 Earth — sun distances from the
star.
Picture distant blue
stars brighter
than the full moon at night, shining through the spidery veins of
dust and gas that hang through the nebula like cobwebs.
«We're not sure whether these
stars are holding onto reservoirs of gas much longer
than expected, or whether there's a sort of «last gasp» of second - generation gas produced by collisions of comets or evaporation from the icy mantles of
dust grains,» said Meredith Hughes, an astronomer at Wesleyan University and coauthor of the study.
These
star - shaped grippers, made of gold - coated nickel and no bigger
than specks of
dust, start out in water in the open position.
Its sensitivity and high resolution — 10 times sharper
than the Hubble Space Telescope — are ideal for observing the «cool» universe, or the regions of gas and
dust around
stars.
This indicates it is a cloud of gas and
dust rather
than a
star, they say, because a
star is so hot that it should be brighter at the shorter wavelength.
The Atacama Large Millimeter / Submillimeter Array (ALMA), high up in the deserts of northern Chile, is sensitive to light from cooler objects of the cosmos: clouds of gas and
dust rather
than burning
stars.
The discovery of jets pushing away from
dust - shrouded protostars at hundreds of miles per second was the first hint to astronomers that
star formation was a far more chaotic process
than they had envisioned.
If the
star is closer
than 1,300 light - years, extinction from gas and
dust in the interstellar medium can not explain the current level of dimming.
Produced by
stars, the
dust causes light to look redder
than it really is when observed visually, which can make it difficult for astronomers studying properties of
stars.
Fear not, wayward hobbits: this is nothing more
than the young
star Formalhaut and its elliptical
dust cloud.
The $ 720 million observatory has surpassed expectations, peering through
dust to see planetary nurseries and cauldrons of young
stars more clearly
than ever before.
Using the Gemini Planet Imager (GPI) at the Gemini South telescope in Chile, the researchers identified a disc - shaped bright ring of
dust around a
star only slightly more massive
than the sun, located 360 light years away in the Centaurus constellation.
Zuckerman and Becklin believe that most of HD 98800's
dust is probably in a thick disc just a few times farther from the
star than the Earth is from the Sun.
New observations of the
star using the SPHERE instrument on the VLT have clearly revealed how the brilliant light of VY Canis Majoris lights up the clouds of material surrounding it and have allowed the properties of the component
dust grains to be determined better
than ever before.
That explains why radio astronomers have found more complex molecules in the warmer, more active
star - birthing regions of
dust clouds
than in the colder, darker areas.
The events included «superflares» of more
than 100 million °C, arcing far into space and striking disks of gas and
dust around the young
stars.
Or, as Joni Mitchell put it in her song «Woodstock» more
than a decade later, «We are
star dust.»
NGC 253, a giant that's somewhat smaller
than the Milky Way, is experiencing a starburst: For its size, it's converting gas and
dust into new
stars at a rapid clip, 2.8 solar masses per year.
But we saw that the dips were deeper in blue [light]
than they were in the red, which indicates that something more transparent, like
dust, is crossing in front of the
star,» Boyajian says.
The pressure of starlight from the
star, which is 23 times more luminous
than the Sun, then expelled the
dust far into space.
In 1983, an orbiting satellite called IRAS discovered far more infrared radiation — which has waves longer
than red light — coming from the Vega
than expected for small interstellar
dust grains found around young, early - type
stars (Harvey et al, 1984).
u A few
stars might be Population III
stars that became polluted with elements heavier
than hydrogen and helium that fell into the
star as
dust.
For example, more
than 30 sets of binary
stars (two
stars orbiting their common center of mass) have one or more planets orbiting each
star.12 The rapidly changing gravity fields produced by each binary
star would have prevented any orbiting cloud of
dust and gas from collapsing into one planet.
These galaxies are enshrouded in
dust at the edge of the universe, and tell us about
star birth more
than 90 % of the way back to the start of time.
This outer
dust is easier to see
than the inner, warm
dust due to its greater distance from the
star.
After surveying nearly 50
stars from 2008 to 2011, scientists have been able to determine with remarkable precision how much
dust is around distant
stars — a big step closer into finding planets
than might harbor life.
Infrared will allow us to observe more closely the infant galaxies,
stars and planets in the
dust of the universe, rather
than the «toddler» ones that Hubble has picked up [source: James Webb Space Telescope].
Among the incredible Hubble cloud images, none has been received with greater public acclaim
than the detailed 1995 snapshot of newborn
stars emerging from giant pillars of gas and
dust inside the Eagle Nebula.
Any more massive
than that and its gravity would destroy the vast
dust belt encircling the
star,» Kalas says.
The disk is fainter
than the
star because its
dust only reflects light.
The leading explanation is that Epsilon Aurigae consists of a yellow giant
star orbited by a normal
star slightly bigger
than the Sun embedded in a thick disc of
dust and gas oriented nearly edge on when viewed from Earth.
Thus, a
star that is 6,000 light - years away in the plane of the Galaxy will appear four times fainter
than it would otherwise were it not for the interstellar
dust.