Like planets,
dust near a star is hard to see.
Some planets are so near their star that they are losing mass too rapidly to have been planets for very long.14 Besides, their rocky cores would have melted before the planet's evolution could begin.15 Others are too far from their star and
the dust near the star needed to grow a planet.
Not exact matches
We can see the
nearest few of these great collections of
stars, gas (mostly hydrogen) and
dust with our eyes from Earth.
But in the
near future ALMA will be able to observe
dust traps closer to their parent
stars, where the same mechanisms are at work.
ALMA discovers cold
dust around
nearest star.»
One such
star with a prominent
dust disk, called Epsilon Eridani, is one of the 10
nearest stars investigated by the HOSTS Survey.
Unlike the Solar System where most of the gravitational pull comes from the Sun and is simple to model, it is much harder to describe the gravitational field
near the centre of the Galaxy, where millions of
stars, vast clouds of
dust, and even dark matter swirl about.
Unlike the famous Sloan Digital Sky Survey, which mapped only part of the sky, the new 2MASS Redshift Survey covers 95 % of surrounding space, skipping over only the region
near the plane of our own galaxy, where the Milky Way's
stars and
dust block the view of remote objects.
The discovery sprang from an observation by NASA's Spitzer Space Telescope, which spotted the infrared glow of a band of
dust near a bright
star called Eta Corvi.
If Breakthrough Starshot launches tiny spacecraft to our
nearest star system at one - fifth light speed, they will have to survive bombardment with interstellar
dust
This unusually compact cloud of
dust and gas
near the center of the Milky Way in the direction of the constellation Sagittarius is energized by a hot young
star at its core, and it's a veritable alphabet soup of molecules.
Ordinary
stars also blow
dust into space when they swell into red giants
near the end of their lives.
The debris field of very fine
dust was likely created from collisions among developing infant planets
near the
star, evidenced by a bright ring of dusty debris seen 7 billion miles from the
star.
Sage also knew that
dust swirling that
near the
star would absorb so much heat over those millions of years that the
dust would vaporize into the vacuum of space, so no planet would form, especially a Jupiter - size planet.15
The Soul Nebula is an open cluster of
stars surrounded by a cloud of
dust and gas over 150 light - years across and located about 6,500 light - years from Earth in the constellation Cassiopeia,
near the Heart Nebula.
Much
dust is visible here, as well as a few pink nebulae, signs of
star formation,
near the end of one of the arms.
Two of these visible - light pictures show interstellar gas and
dust around young
stars at the beginning of their lives, and two more show gas ejected from old
stars that are
nearing the end of theirs.
If located within a few AUs of the central
star, this
dust is warmed to temperatures that produce
near - infrared emission and small grains produce scattered light.
We aim to determine the level of
near - infrared exozodiacal
dust emission around a sample of 42 nearby main sequence stars with... ▽ More (Abridged) Dust is expected to be ubiquitous in extrasolar planetary systems owing to the dynamical activity of minor bod
dust emission around a sample of 42 nearby main sequence
stars with... ▽ More (Abridged)
Dust is expected to be ubiquitous in extrasolar planetary systems owing to the dynamical activity of minor bod
Dust is expected to be ubiquitous in extrasolar planetary systems owing to the dynamical activity of minor bodies.
Our overall detection rate is 18 %, including four new detections, among which are... ▽ More The HOSTS (Hunt for Observable Signatures of Terrestrial Systems) survey searches for
dust near the habitable zones (HZs) around nearby, bright main sequence
stars.
We aim to determine the level of
near - infrared exozodiacal
dust emission around a sample of 42 nearby main sequence
stars with spectral types ranging from A to K and to investigate its correlation with various stellar parameters and with the presence of cold
dust belts.
Abstract: The HOSTS (Hunt for Observable Signatures of Terrestrial Systems) survey searches for
dust near the habitable zones (HZs) around nearby, bright main sequence
stars.
Interferometric observations obtained with the VLTI and the KIN have identified
near - and mid-infrared excesses attributed to hot and warm exozodiacal
dust in the inner few AU of the
star.
On June 16, 2010, the Hubble Heritage Project released a very detailed, composite image of the dark lanes of
dust crisscrossing the giant elliptical galaxy Centaurus A. Taken on July 10, 2010 with the Hubble Space Telescope's Wide Field Camera 3, the panchromatic image of ultraviolet through
near - infrared wavelengths shows new details such as bluish clusters of young massive
stars and reddish gas nebulae undergoing
star birth normally obscured by
dust.