Because it is above the atmosphere, the Hubble Space Telescope can detect these small dead stars in nearby
old star clusters called globular clusters.
«No single model for the formation of these star clusters can currently reproduce the diversity of structural properties we have observed for
old star clusters,» Professor Forbes said.
47 Tucanae is a 12 - billion - year -
old star cluster located 13,000 light - years from Earth in the southern constellation of Tucana the Toucan.
According to the researchers, this particular IMBH is located in the center of a 12 billion - year -
old star cluster named 47 Tucanae, where its gravity is affecting the motion of stars.
Cosmically speaking, the the 500,000 - year -
old star cluster is extremely young.
The stars which are even older have dissipated into a more diffuse background; this includes intermediate population I stars,
older star clusters and the younger representatives of the planetary nebulae.
Not exact matches
Star clusters are made up of giant circular clouds of
old stars, some around 12 billion years
old (the universe itself is 14.8 billion years
old), that clump together due to gravity, and are found circling cores of galaxies.
Yet recent discoveries of young
stars in
old globular
clusters have scrambled this tidy picture.
When the cosmos was a few hundred million years
old, this gas coalesced into the earliest
stars, which formed in
clusters that clumped together into galaxies, the
oldest of which appears 400 million years after the universe was born.
While globular
clusters are billions of years
old, the planetary nebula phase of a
star's life only lasts for a few thousand years, so it's exceedingly rare to find them in globulars.
This image clearly shows
stars nearly all the way into the core, and you can see that many of the
stars are red, indicating their great age: The
cluster is over 10 billion years
old.
Population II
stars are
older, with a low heavy - element content, and are found in the Milky Way Bulge and Halo, and globular
star clusters.
Conventional wisdom says that globular
star clusters are the stodgy
old codgers of the universe, but it turns out that many of these
clusters are young
The group of bright blue - white
stars at the upper - left is the Trapezium
Cluster — made up of hot young
stars that are only a few million years
old.
At that time, the sun likely resembled Iota Horologii, because the
star is young: it's thought to have escaped from the Hyades
star cluster, which is just 600 million years
old, or about one - eighth our sun's present age.
On the other hand globular
clusters are much bigger spherical collections of much
older stars that orbit around the centre of a galaxy.
These
stars may even be the remains of the most massive and
oldest surviving
star cluster of the entire Milky Way.
The NASA / ESA Hubble Space Telescope has captured the best ever image of the globular
cluster Messier 15, a gathering of very
old stars that orbits the centre of the Milky Way.
Not only are these
stars powerful evidence for an important theory of galactic evolution, they are also likely to be over 10 billion years
old — the dim, but dogged survivors of perhaps the
oldest and most massive
star cluster within the Milky Way.
As RR Lyrae
stars typically reside in ancient stellar populations over 10 billion years
old, this discovery suggests that the bulging centre of the Milky Way likely grew through the merging of primordial
star clusters.
As this
cluster is relatively
old, a part of this lost mass will be due to the most massive
stars in the
cluster having already reached the ends of their lives and exploded as supernovae.
RR Lyrae
stars allow exact distance estimations and are found only in stellar populations more than 10 billion years
old, for example, in ancient halo globular
clusters.
Although in the case of NGC 2477 astronomers seem to have underestimated the age of the
cluster; they may have overestimated the age of other
clusters, and this may explain the conflict between the ages of the
oldest stars and the latest estimate of the Universe's age.
Stars in the extremely old globular cluster NGC 6397 are slightly polluted by the shattered fusion products of an even earlier generation of s
Stars in the extremely
old globular
cluster NGC 6397 are slightly polluted by the shattered fusion products of an even earlier generation of
starsstars.
He calculated that the
oldest stars in the galactic center had to be at least one billion years
older than the
oldest stars in globular
clusters to allow enough time for so many RR Lyraes to evolve there.
Some
stars in globular
clusters may be 15 billion years
old, he says, but the great bulge at the center of the Milky Way — a younger part of the galaxy, according to conventional wisdom — actually holds
stars that are 1 or 2 billion years
older.
Because globular
clusters are the
oldest known structures in the universe, the beryllium must have been produced by the long - sought first generation of
stars.
Ask most astronomers where to find the
oldest stars in the galaxy and they'll tell you to look at globular
clusters, dense knots of
stars that hover above and below the plane of the Milky Way.
Lee doesn't dispute that globular
cluster stars are
old — only that they are the
oldest.
By that logic, globular
clusters — swarms of metal - poor
stars as
old as our galaxy — are the last place one would expect to find planets.
The
cluster contains thousands of
stars less than 2.5 million years
old, making it the best place to find the biggest young
stars that have not yet exploded.
Formed a billion years after the Big Bang, the universe's
oldest and most distant known planet circles a collapsed
star, or pulsar (green circle), in the globular
cluster M4, which is 5,000 light - years away from Earth.
Globular
clusters are spherical clumps of hundreds of thousands of
old, low - mass
stars, held together by the mutual pull of their gravity.
In a new study, the scientists show their theoretical predictions last year were correct: The historic merger of two massive black holes detected Sept. 14, 2015, could easily have been formed through dynamic interactions in the
star - dense core of an
old globular
cluster.
Now, scientists have shown that there's some truth to the age -
old advice: A dimming of the Pleiades
star cluster may actually auger a weather change that affects local farmers, according to a report in today's Nature.
If this result is confirmed, it means that our Galaxy may have looked different in the past with more globular
clusters — tightly packed conglomerations of hundreds of thousands of
old stars — than the 150 to 200 that it has today.
But the
star cluster has to be very dense and very young — about 10 million years
old — to allow this to happen, say the researchers.
The team suggests that they are rather evolved,
old members of the
cluster consuming the last of their gas to form
stars.
Brighter
stars also live shorter lives, and since globular
clusters are
old, those
stars have died out.
The
cluster is more than 12 billion years
old, which means the
stars that the researchers looked at formed only a few hundred million years after the death of first - generation
stars.
Globular
clusters, which are found in the halo of a galaxy, contain considerably more
stars and are much
older than the less dense galactic, or open
clusters, which are found in the disk.
The Milky Way's dense globular
clusters are spherical swarms of red, lightweight and ancient
stars, most of them more than 10 billion years
old.
This would be fine, were it not for the fact that studies of globular
clusters of
stars suggests they are about 15 billion years
old.
STScI / NASA press releases: Hubble Makes the First Precise Distance Measurement to an Ancient Globular
Star Cluster Hubble Unmasks Ghost Galaxies Deepest View of Space Yields Young
Stars in Andromeda Halo Hubble Identifies Source of Ultraviolet Light in an
Old Galaxy ESA press releases: Hubble Unmasks Ghost Galaxies Four Unusual Views of the Andromeda Galaxy Public speaking: On the Trail of the Missing Galaxies High - Level Science Products from Large and Treasury Programs: GO - 9453: The Age of the Andromeda Halo (126 orbits) GO - 10265: The Formation History of Andromeda (107 orbits) GO - 10816: The Formation History of Andromeda's Extended Metal - Poor Halo (128 orbits) GO - 11664 / 12666: The WFC3 Galactic Bulge Treasury Program: Populations, Formation History and Planets (56 orbits) GO - 12549: The Formation History of the Ultra-Faint Dwarf Galaxies (113 orbits)
«
Old, compact
star clusters, such as globular
clusters, are well known to amateur astronomers,» Professor Forbes said.
The group of bright blue - white
stars at the left is the Trapezium
Cluster, hot young
stars that are only a few million years
old.
NGC 6997 is definitely a
star cluster, but it is rather
old and it probably did not form in the nebula.
Gillian Wilson, professor of physics and astronomy at UC Riverside, added, «Fascinatingly, however, the study found that the percentage of galaxies which had stopped forming
stars in those young, distant
clusters, was much lower than the percentage found in much
older, nearby
clusters.
Others, known as globular
clusters, are among the
oldest objects in the Universe and contain up to a million ancient
stars.
This scenario is supported by the age estimations of the
stars in the inner halo (10 — 12 billion years
old) and globular
clusters.