HUGE gas reservoirs have been spotted
around distant galaxies, where they can fuel new stars — contrary to what we thought.
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).
Not exact matches
A look at the universe and all its wonders — from our neighborhood
around the sun to the most
distant galaxy, and beyond.
Some research has been done to deduce the chemical makeup of very early
galaxies, based on observations of very bright,
distant galaxies, or of very old stars that formed in the early universe and are still
around today, Hewitt said.
«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.
It has been used to detect planets
around distant stars within the Milky Way
galaxy, and was among the first methods used to confirm Albert Einstein's general theory of relativity.
Albert Einstein's theory predicts that the gravitational effects of the nearer
galaxy bends the light of the more
distant one
around it, a process called gravitational lensing.
Every 12 years, a black hole at the centre of a
distant galaxy completes an orbit
around an even bigger black hole, marking this with a violent outburst
But
around the same time studies of very
distant galaxies, which we see as they were when the Universe was very young, were setting constraints on the amount of baryonic matter in the Universe (New Scientist, Science, 30 April).
Remarkably, the distribution of star - forming
galaxies around a cluster of
galaxies in the more
distant universe (5 billion years ago) corresponds much more closely with the weak lensing map than a slice of the more nearby universe (3 billion years ago).
The bluish circle
around the
galaxies is the light from a more
distant galaxy bending
around the cluster's center due to gravity from both stars and dark matter.
The source was traced to a
distant galaxy, so far away that its light took
around 3.9 billion years to reach Earth.
In theory, very
distant (and therefore young)
galaxies should have weaker magnetic fields than
galaxies which are
around today.
The GMT aims to discover Earth - like planets
around nearby stars and the tiny distortions that black holes cause in the light from
distant stars and
galaxies.
That means that if we were on those far
distant galaxies — right this second — looking at Earth with a powerful telescope, we'd be watching the dinosaurs trample
around our planet.
When a very massive
galaxy comes smack in between Earth and a
distant galaxy, the light from the
distant galaxy is bent
around the huge impediment.
Capable of observing the Universe by detecting light that is invisible to the human eye, ALMA will show us never - before - seen details of the birth of stars, infant
galaxies in the early Universe, and planets coalescing
around distant suns.
A
galaxy could be used as magnifying glass as light from a
distant galaxy is warped
around the closer object.
This material gathers into huge turbulent reservoirs of cool, low - density gas, extending more than 30 000 light - years from the
galaxy's star forming region [3] These turbulent reservoirs of diffuse gas may be of the same nature as the giant glowing haloes seen
around distant quasars..
The light of a
distant galaxy is re-directed
around this core, often producing multiple images of the background
galaxy (see the image above for an example).
Indeed, GRBs appear to emit produce even more energy than supernovae or even quasars (which are energetically bright accretion disks and bi-polar jets
around supermassive black holes that are most commonly found in the active nuclei of some
distant galaxies and possibly even in the pre-galaxy period after the Big Bang).
Researchers have, to an extent, been able to work
around this impediment using a variety of differing observational techniques paired with insight gained from studies of
distant spiral
galaxies, in order to develop a basic model of our
galaxy.