In addition, the gravitational lensing of quasars
by distant galaxies is only possible if the lensed quasars are farther away than the galaxy bending the quasar's light.
«Not only did we detect radio signals emitted
by distant galaxies when the Universe was three billion years younger, but their gas reservoirs turned out to be unexpectedly large, about 10 times larger than the mass of hydrogen in our Milky Way.
A radical new model of gravity seems to account for bending of light
by distant galaxies without invoking extra unseen mass whose identity remains mysterious
Measuring the atomic hydrogen signal emitted
by distant galaxies is one of the main scientific drivers behind the billion dollar Square Kilometre Array (SKA) project, for which technology demonstrators like the Australian SKA Pathfinder are under construction.
They match Einstein's explanations of everything from the bending of light
by distant galaxies to the distortion of time in those gps satellites.
Story number 2: Astronomers have detected an energetic outburst near the constellation Sagittarius that they believe was caused
by a distant galaxy in the midst of reversing the direction of its spiral rotation.
Not exact matches
It would be otiose to give examples: a
distant thunder is in the past as much as a
distant star; but no matter how far in time - space a star or
galaxy is, it is always faintly immanent in my Here - Now even when its action is below the threshold of human perception; its action can be made visible
by a combination of lenses or a prolonged photographic exposure.
Today astronomers measure how much dark matter a cluster of
galaxies may have
by observing how the cluster bends light from more
distant objects.
Chemical calculations show that helium hydride should be visible in clouds around
distant galaxies and supernovas, or even in modern planetary nebulas (shells of gas expelled
by aged, sunlike stars).
By the 1930s, American astronomers Vesto Melvin Slipher and Edwin Hubble had measured the movement of
distant galaxies, convincing everyone — even Einstein — that the universe was expanding, despite it all.
MAGNIFYING THE COSMOS The light from a
distant galaxy (lower right) is warped
by the gravity of a closer, massive
galaxy (bright blur in center).
These can reveal
distant, ancient
galaxies whose light has been stretched
by the universe's expansion to more than triple its initial wavelength.
When dark matter lies between us and a
distant galaxy, the light of the
galaxy can be warped
by the gravity from the dark matter.
If the expansion is slowing down, the velocity of a
distant galaxy would be relatively greater than the velocity predicted
by Hubble's law.
The instrument is sensitive to near - infrared light, the wavelengths at which the emissions of extremely
distant galaxies — stretched
by the expansion of space — shine most brightly.
Astronomers studying
distant galaxies powered
by monster black holes have uncovered an unexpected link between two very different wavelengths of the light they emit, the mid-infrared and gamma rays.
To locate the source, a group directed
by Puget and David L. Clements in Paris has started the first far - infrared search for
distant galaxies, using the European Space Agency's Infrared Space Observatory (ISO).
A team of astronomers, led
by Karina Caputi of the Kapteyn Astronomical Institute at the University of Groningen, has now unearthed many
distant galaxies that had escaped earlier scrutiny.
Christian Marinoni and Adeline Buzz at the University of Provence in Marseille, France, realised they could fine - tune such estimates
by observing
distant galaxy systems in which two
galaxies orbit each other.
Guyon adds that the system will help astronomers to study the skies more efficiently,
by bringing large objects, such as nearby
galaxies, into focus all at once, and
by allowing more
distant objects to be studied in a single snapshot.
To find out, they studied
distant galaxies whose light has been distorted
by the gravitational pull of other, nearer
galaxies.
According to recent measurements
by a Nobel prizewinning team, space is stretching 9 per cent faster than we think it should be — yanking
distant galaxies away from us at a rate that defies easy explanation.
This was the conclusion announced in March
by astronomers who studied explosions of stars in
distant galaxies.
Submillimeter emissions are typically produced
by carbon and water molecules in
distant galaxies and star - forming regions.
The other method, practised
by Riess and his colleagues, measures how
distant galaxies appear to recede from us as the universe expands, using stars and supernovae of known brightness to gauge the distance to those
galaxies.
Using the Very Large Array of the National Radio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a
distant galaxy and found that it would have contained billions of young, massive stars surrounded
by clouds of hydrogen gas.
These arced or blobby features, seen in images of deep space, are actually
distant galaxies whose light has been bent
by the mass of foreground
galaxies.
The team made a 3 - D map
by collecting light from over 70,000
galaxies, peering all the way into the
distant universe, and
by using this light to measure how far these
galaxies are from our own Milky Way.
Getting a high - resolution spectrum was possible thanks to a fortunate trick of nature: The light of the
distant object is magnified 50 times
by the gravity of a
galaxy cluster halfway between the Earth and cB58.
These gamma - ray bursts, astrophysicists recently learned, originate in
distant galaxies and are unfathomably powerful — as much as 10 quadrillion (a one followed
by 16 zeros) times as energetic as the sun.
Similarly, centrifugal forces are caused
by rotation relative to the
distant galaxies, so in principle you could produce centrifugal forces
by standing still and making the Universe rotate about you.
Researchers estimated the rate of star formation
by measuring far - infrared wavelengths of light emanating from the
distant galaxy.
However, through the phenomenon known as «gravitational lensing,» a massive, foreground cluster of
galaxies acts as a natural «zoom lens» in space
by magnifying and stretching images of far more
distant background
galaxies.
When you see Jupiter shining in the night sky, for example, you're looking about an hour back in time, whereas the light from
distant galaxies captured
by telescopes today was emitted millions of years ago.
The objects causing these low - frequency ripples — such as orbiting supermassive black holes at the centers of
distant galaxies — would be different from the higher frequency ripples, emitted
by collisions of much smaller black holes, that have so far been detected on Earth.
The light waves from
distant galaxies are stretched and reddened
by the expansion of the universe, and this redshift is proportional to a
galaxy's distance.
It said that everything that happens in the cosmos at large — be it an apple falling from a tree on Earth or the
distant whirling of a cluster of
galaxies — happens because stuff follows invisible contortions in space and time that are caused
by the presence of other stuff.
The CIB glow is more irregular than can be explained
by distant unresolved
galaxies, and this excess structure is thought to be light emitted when the universe was less than a billion years old.
The study led
by Donahue looked at far - ultraviolet light from a variety of massive elliptical
galaxies found in the Cluster Lensing And Supernova Survey with Hubble (CLASH), which contains elliptical
galaxies in the
distant universe.
Many
distant quasars — luminous
galaxies, thought to be powered
by large central black holes — are known to contain warm dust, which glows at infrared wavelengths.
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.
Five
distant galaxies so choked with dust that they are completely invisible at optical wavelengths have been spotted at submillimetre wavelengths
by the European Space Agency's Herschel telescope.
«Till recent years, in the paradigm of
galaxy formation and evolution, elliptical
galaxies were thought to have formed
by the merging of stellar disks in the
distant Universe.
If a
distant galaxy were lined up right behind one more close
by, this warping would bend and magnify the faraway
galaxy's image, a phenomenon now called gravitational lensing.
Looking at a
distant galaxy: the radio chart (left) shows the image of the blazar PKS 1830 - 211 distorted
by the gravitational lens effect.
New research
by Harvard astronomers Peter Williams and Edo Berger shows that the radio emission believed to be an afterglow actually originated from a
distant galaxy's core and was unassociated with the fast radio burst.
The start of a jet in the
distant galaxy J1415 +1320 was magnified
by a massive object in the foreground, closer to Earth.
Astronomers have uncovered a supermassive black hole that has been propelled out of the center of a
distant galaxy by what could be the awesome power of gravitational waves.
Supernova measurements indicate that
distant galaxies are separating from one another
by 73 kilometers per second for each megaparsec (about 3.3 million light - years) of distance between them.
An international team of astronomers, led
by Imperial College London, used a new way of combining data from the two European Space Agency satellites, Planck and Herschel, to identify more
distant galaxy clusters than has previously been possible.