Not exact matches
Physicists still puzzle over what makes up dark energy, along with another unexplained cosmic constituent, dark matter, an additional kind of
mass that must exist to explain observations of
how galaxies and
galaxy clusters rotate.
They found that the
mass in the central bulge (regardless of
how big the disk surrounding it may be) is the key to knowing the colour of the whole
galaxy.
«This
mass range gets interesting, because these «ultra-faint» dwarf
galaxies are so faint that we do not yet have a complete observational census of
how many exist around the Milky Way.
By measuring
how the light bent, astronomers can measure the
galaxy's
mass.
Tipping the scales at less than about a million suns in
mass, middleweight black holes may hold clues to
how their much larger siblings, and
galaxies, first formed
Astronomers can measure a
galaxy's
mass by
how stars move within it: The faster they move, the more massive it is.
In terms of
mass they lie between the more commonly found stellar -
mass and supermassive types of black hole [3], and could tell us about
how black holes grow and evolve within clusters like Messier 15, and within
galaxies.
* This technique, known as integral field spectroscopy, allows astronomers to simultaneously study the properties of different parts of an object such as a
galaxy to see
how it is rotating and to measure its
mass.
Gaining a better understanding of
how much
mass black holes accrete may therefore provide new insight on
how galaxies pack on the pounds, astronomers note.
The team also compared the
masses of the black holes with the total
masses of their host
galaxies to determine
how much matter they had swallowed.
«What we'd really like is to know
how common
galaxies of different
masses were at different ages of the universe,» he says.
Two teams of astronomers led by researchers at the University of Cambridge have looked back nearly 13 billion years, when the Universe was less than 10 percent its present age, to determine
how quasars — extremely luminous objects powered by supermassive black holes with the
mass of a billion suns — regulate the formation of stars and the build - up of the most massive
galaxies.
Astronomers made the new
mass estimate by watching
how strongly the gravity of the
galaxy cluster distorted the light of objects behind it.
Astronomers have found more than 1,000 «low - surface - brightness»
galaxies over the past decade, significantly altering our views of
how galaxies evolve and
how mass is distributed in the universe
«The neural networks we tested — three publicly available neural nets and one that we developed ourselves — were able to determine the properties of each lens, including
how its
mass was distributed and
how much it magnified the image of the background
galaxy,» said the study's lead author Yashar Hezaveh, a NASA Hubble postdoctoral fellow at KIPAC.
Within the lensed image of the source are small - scale distortions, which encode an imprint of
how the lens
galaxy's
mass is distributed.
To find out
how they became so sparse, van Dokkum and his colleagues tracked
how fast the stars in Dragonfly 44 move around the
galaxy, and so calculated its
mass: a faster speed means a more massive
galaxy.
By analyzing this time difference and by measuring
how fast the material is moving around the center of the
galaxy, they were able to determine the
mass of this central black hole.
The knowledge of
how exactly stars in a
galaxy or a star cluster are distributed by
mass is crucially important for astronomers.
The detection of Refsdal's reappearance served as a unique opportunity for astronomers to test their models of
how mass — especially that of mysterious dark matter — is distributed within this
galaxy cluster.
By cross-correlating large - scale surveys of
galaxies and observations of
how galaxies distort background light in a relativistic process known as weak lensing, Ferreira says, the true nature of
mass and the forces acting on it can be tested.
Supermassive black holes more than a million times the
mass of our sun exist at the centers of many
galaxies, but
how they came to be is unclear.
Studying more objects like «Oumuamua will enable us to work out
how much debris is left over from star formation and
how much this adds to the
mass of our
galaxy.
They followed the motion of 10 star clusters to work out
how much
mass the
galaxy had.
Scientists can figure out
how much
mass there is in a
galaxy by tracking
how fast things inside move, Pieter van Dokkum, one the authors of a new research paper published in Nature, told Newsweek.
By studying different models of just
how mass is positioned in the
galaxy cluster, astronomers could predict one more light path for Refsdal, one that would delay the light reaching the telescope until late 2015 or early 2016.
Using luminosity measurements, he determined
how much
mass should be in the cluster and then, because
mass and gravity are related, calculated
how fast the
galaxies should be moving.
The more luminous a
galaxy, the more
mass it possesses (see
How Stars Work).
The goal of the observations is to constrain
how the star formation assembled the bulk of the stellar
mass in today's massive
galaxies and
how secular processes crystallised the Hubble sequence around z ~ 1.
The
mass is estimated by looking at
how the
galaxy rotates, as well as its spectrum using spectroscopy.
Once a
galaxy's
mass is determined, the other tricky thing is figuring out
how much of that
mass is made of stars.
The detection of this fifth appearance of the Refsdal supernova served as a unique opportunity for astronomers to test their models of
how mass — especially that of mysterious dark matter — is distributed within this
galaxy cluster, and they seem to be right on track.
In an effort to learn more about dark matter, astronomers observed
how galaxy clusters collide with each other — an event that could hold clues about the mysterious invisible matter that makes up most of the
mass of the universe.
As Thanos smiles and stares out over a sunrise, at peace with his devastating decision to commit
mass slaughter in order to prevent the
galaxy's resources from being used up via overpopulation, it's difficult not to wonder
how Marvel would resurrect some of these characters, not to mention have them battle back against the despotic conqueror.