Astronomers have long debated whether
such early galaxies could have provided enough radiation to warm the hydrogen that cooled soon after the big bang.
It is very surprising and it is the first time that dust has been found in
such an early galaxy.
Not exact matches
Gal - Yam thinks the conditions in the host
galaxy could be like those in the
early universe, when theory says
such giant stars were born and died in great numbers, seeding the universe with heavy elements.
Such views suggest that tiny
galaxies in the
early universe played a crucial role in cosmic reionization — when ultraviolet radiation stripped electrons from hydrogen atoms in the cosmos.
Finding so many primordial
galaxies allows scientists to pin down crucial questions about the newborn universe,
such as when light from
early stars and
galaxies penetrated the
early cosmic gloom.
Marijn Franx, a member of the team from the University of Leiden highlights: «The discovery of GN - z11 was a great surprise to us, as our
earlier work had suggested that
such bright
galaxies should not exist so
early in the Universe.»
Finding
such a
galaxy early in the history of the universe challenges the current understanding of how massive
galaxies form and evolve, say researchers.
«Among other things,» he writes, «I learned that merging
galaxies can fire up to ultraluminous status
early in the encounter, against the prevailing wisdom that put
such activity only late in the final merger stage.»
«To find
such an event in
early type
galaxies where star formation is rare is an incredibly fortunate find.
He did not expect to find any massive
galaxies earlier than about 9 billion years ago because theoretical models predict that
such large objects form last.
Conroy suspects that violent conditions in the
early universe —
such as
galaxy mergers — shocked and compressed gas and dust in particular areas, creating agglomerations of thousands of stars in particular areas.
Earlier research from Hubble's Cosmic Origins Spectrograph (COS)- Halos program studied 44 distant
galaxies and found halos like Andromeda's, but never before has
such a massive halo been seen in a neighboring
galaxy.
GREEN
GALAXIES Galaxies in the early universe emitted lots of green light, such as seen in this nebula (NGC 6826) in the Mi
GALAXIES Galaxies in the early universe emitted lots of green light, such as seen in this nebula (NGC 6826) in the Mi
Galaxies in the
early universe emitted lots of green light,
such as seen in this nebula (NGC 6826) in the Milky Way.
Also, as pointed out by Turner
earlier this year, an older Universe gives the favoured cold dark matter model time to make the large collections of
galaxies seen today, without bringing in any other «fixes»,
such as the addition of hot dark matter (New Scientist, Science, 16 July).
Several ground - based microwave telescopes,
such as the South Pole Telescope, are tracking how the structure of very distant
galaxy clusters grew in the
early Universe under the influence of gravity.
Supermassive black holes in the cores of
galaxies are thought to fatten slowly over eons, so finding
such a heavyweight so
early in the history of the universe is «really pushing it,» he says.
On the other hand, if there are 100 billion suitable planets in our
galaxy, if the origin of life is highly probable, if there are billions of years of evolution available on each
such planet and if even a small fraction of technical civilizations pass safely through the
early stages of technological adolescence, the number of technological civilizations in the
galaxy today might be very large.
«We can explore
such original
galaxies in full detail and probe the conditions of the
early universe,» said Ignacio Trujillo, of the Instituto de Astrofisica de Canarias at the University of La Laguna, Spain.
Now the researchers hope that future observations of a large number of distant
galaxies using the ALMA telescopes could help unravel how frequently
such evolved
galaxies occur in this very
early epoch of the history of the universe.
The proximity of UGC 1382 will be a boon to revealing other features of
such elusive giants in addition to understanding other seemingly normal
early galaxies.
What the team directly observed was the last wave of Population III stars, suggesting that
such stars should be easier to find than previously thought: they reside amongst regular stars, in brighter
galaxies, not just in the
earliest, smallest, and dimmest
galaxies, which are so faint as to be extremely difficult to study.
Astronomers believe that
such collisions between
galaxies were common in the
early universe when
galaxies were closer together.
Because distances between
galaxies are so vast today,
such mergers were thought to be rare.36 But the Hubble telescope, in its furthest look back in time, has photographed dozens of
galaxies in the process of colliding.37 Obviously,
galaxies formed quickly in the
early, much more compact universe.
Such studies are important in understanding how the Universe evolved from an
early dark period to one when
galaxies began to shine.
Such a view would yield a treasure trove of information from which to deduce the
early history of structure formation, and the origin of the stars,
galaxies, clusters and quasars that we see today.
Because the discovery of
such an
early source with powerful Lyman - alpha is somewhat unexpected, it provides new insight into the manner by which
galaxies contributed to the process of reionization.
The question astronomers have been asking is whether
such starbursts in the
early universe were the result of having an overabundant gas supply, or whether
galaxies converted gas more efficiently.
Scientists have decoded faint distortions in the patterns of the universe's
earliest light to map huge tubelike structures invisible to our eyes - known as filaments - that serve as superhighways for delivering matter to dense hubs
such as
galaxy clusters.
«Until ALMA, we've never been able to see the formation of
galaxies in
such detail, and we've never been able to measure the movement of gas in
galaxies so
early in the Universe's history,» said co-author Stefano Carniani, from Cambridge's Cavendish Laboratory and Kavli Institute of Cosmology.
Such computers can help discover planets and
galaxies, diagnose diseases, and do many tasks
earlier than usual.