The same scenario may hold for
the distant faint galaxies that astronomers discovered before they saw LSBs in large numbers.
Not exact matches
Astronomers exploit this property of space to use the clusters as a zoom lens to magnify the images of far - more -
distant galaxies that otherwise would be too
faint to be seen.
Along with the familiar cosmic microwave background — the afterglow of the big bang — the
distant universe is suffused with an infrared background, thought to come from
galaxies and stars too
faint and far away to see.
LIGHTEN UP Some of the
faintest, most
distant galaxies detected to date (arcs) appear in this Hubble Space Telescope image of the massive
galaxy cluster Abell 2744.
«You build bigger, you go
fainter, you go deeper, and you'll have a shot at a major discovery,» explains Pudritz, «So building these larger machines will no doubt allow us to study the birth of the first
galaxies and even planet formation around
distant stars.
However, such a simple task becomes increasingly hard as astronomers attempt to count the more
distant and
fainter galaxies.
The inset is an image of an extremely
faint and
distant galaxy that existed only 400 million years after the big bang.
The
faint radiation was visible thanks to a fortuitous cosmic alignment: The light from the
distant quasar is amplified by the gravity of a much closer, invisible
galaxy.
But beyond redshift 0.7 (roughly six billion light years
distant),
galaxies become
fainter and more difficult to see.
Looking into the
distant, early universe, we would expect dwarf
galaxies to be numerous but also too
faint to see.
Distant blasts could also help pinpoint the locations of
faint GRB host
galaxies that could be detected by space telescopes like the soon - to - be-refurbished Hubble Space Telescope or NASA's infrared James Webb Telescope, which is set to launch in 2013.
Together, the telescopes create a virtual dish 9000 kilometers wide that can detect the
faintest radio emissions from
distant galaxies.
The imaging data demonstrated that these sources are strongly lensed by foreground
galaxies, which increases their apparent luminosities by a factor of ~ 10, which translates to a savings in telescope time of ~ 100, and allows such
distant and intrinsically
faint objects to be more easily detected.
Researchers were able to confirm characteristics of the Little Cub
galaxy using Keck Observatory's Low Resolution Imaging Spectrograph, a
faint - light instrument capable of taking spectra and images of the most
distant known objects in the universe.
This is a nighttime image of our Milky Way
galaxy, which includes a view of M31, that lies 2.5 million light - years
distant and looks like a
faint spindle, several times the diameter of the full Moon (Image: NASA / STScI)
The gravitational lensing can also sometimes magnify the light of an otherwise too -
faint, very
distant galaxy enough for us to see it — a bonus natural telescope!
Unexpectedly
faint Type 1a supernovae in
distant galaxies led to the 1998 discovery of the accelerating expansion of the universe, on account of dark energy.
Hubble's latest discovery of 250
faint galaxies — formed 600 million to 900 million years after the Big Bang — in the early universe using three
galaxy clusters to magnify the light given off by these
distant objects.
«You can see bulges in
distant galaxies, but you can not resolve the very
faint stars, such as the white dwarfs.
Galaxy clusters enable us to see
fainter light from
galaxies in the
distant universe.
The HDF observation was designed to detect very
faint light from the most
distant galaxies Hubble can observe.
With only a relatively minor change to the observing strategy, taking extra care to avoid extra glare from bright foreground light from the Earth, we enabled the Frontier Fields to see ever
fainter and more
distant galaxies than otherwise would have been possible.
This five - ton instrument was designed to study the most
distant,
faintest galaxies, said UCLA physics and astronomy professor Ian McLean, co-project leader on MOSFIRE and director of UCLA's Infrared Laboratory for Astrophysics.
In
faint,
distant galaxies, the task is dramatically more difficult, but COSMOS - 1908 was one case for which Sanders was able to apply the «robust» method commonly applied to nearby
galaxies.
Knowing the abundance of oxygen in the
galaxy called COSMOS - 1908 is an important stepping stone toward allowing astronomers to better understand the population of
faint,
distant galaxies observed when the Universe was only a few billion years old, Shapley said.
A new analysis of
galaxy colors, however, indicates that the farthest objects in the deep fields must be extremely intense, unexpectedly bright knots of blue - white, hot newborn stars embedded in primordial proto -
galaxies that are too
faint to be seen even by Hubble's far vision — as if only the lights on a
distant Christmas tree were seen and so one must infer the presence of the whole tree (more discussion at: STScI; and Lanzetta et al, 2002).
RESEARCHERS HAVE SOLVED a 60 - year - old mystery regarding the origin of the heaviest elements in nature, conveyed in the
faint starlight from a
distant dwarf
galaxy.
Unfortunately, however, no single SFR estimator is universally available or even applicable in all circumstances: the numerous
galaxies found in deep surveys are often too
faint (or too
distant) to yield significant detections with most standard SFR measures, and until now there have been no global, multi-band observations of nearby
galaxies that span all the conditions under which star - formation is taking place.
It takes highly sensitive (expensive) cameras to capture the
faint light of, say, a
distant galaxy.
This is so narrow, just a few foreground stars in our Milky Way
galaxy are visible and are vastly outnumbered by the menagerie of far more
distant galaxies, some nearly as
faint as 30th magnitude, or nearly four billion times
fainter than the limits of human vision.
The images of the Cartwheel
Galaxies reveal many faint, more distant galaxies, which form a large superstructure and lie near the Sculptor Wall, an enormous structure of galaxy clusters that extends outwards for more than a billion of ligh
Galaxies reveal many
faint, more
distant galaxies, which form a large superstructure and lie near the Sculptor Wall, an enormous structure of galaxy clusters that extends outwards for more than a billion of ligh
galaxies, which form a large superstructure and lie near the Sculptor Wall, an enormous structure of
galaxy clusters that extends outwards for more than a billion of light years.