The Sombrero lies at the southern edge of the rich Virgo cluster of galaxies and is one of the most
massive objects in that group, equivalent to 800 billion suns.
Standing outside one of
these massive objects in the universe, for instance, there's only darkness — the black hole's gravity is so strong that not even light escapes.
The galaxy, EGS - zs8 - 1, was originally identified based on its particular colors in images from Hubble and Spitzer and is one of the brightest and most
massive objects in the early universe.
So - called intermediate - mass black holes fill a gap in astronomer's knowledge of the most
massive objects in the universe.
The Earth and moon can serve as giant detectors for ripples in the fabric of space - time known as gravitational waves, which are given off by stars, black holes and other
massive objects in deep space, researchers say.
General relativity predicts that two
massive objects in a tight orbit around each other will spiral in, slowly at first and then faster until they merge, distorting space - time in perturbations that ripple in all directions.
Despite this, gravity has an influence over huge distances and is the driving force behind the motions of the most
massive objects in the cosmos.
Black holes —
massive objects in space with gravitational forces so strong that not even light can escape them — come in a variety of sizes.
Einstein had proposed in 1915 that gravity would cause light to bend around
massive objects in space, such as stars or galaxies.
That means
massive objects in space can act as lenses, focusing the light from objects even farther from Earth.
Giant clouds of molecular gas — the most
massive objects in our galaxy — are the birthplaces of stars.
Galaxy clusters are the most
massive objects in the universe, containing hundreds to thousands of galaxies, bound together by gravity.
It is one of the brightest and most
massive objects in the early universe.
Much as hair collects around a bathtub drain, the most
massive objects in the Milky Way tend to spiral downward toward the center.
They tell us that there is a central,
massive object in the outflow origin, with a surrounding accretion disc.»
The most
massive object in our immediate vicinity, named The Great Attractor, helps bring matter toward it, while helping make voids even emptier.
The start of a jet in the distant galaxy J1415 +1320 was magnified by
a massive object in the foreground, closer to Earth.
Dawn spent nearly 14 months orbiting Vesta, the second most
massive object in the main asteroid belt between Mars and Jupiter, from 2011 to 2012.
The material circles
the massive object in an accretion disk before being pulled into it.
Not exact matches
When a small
object orbits a big
object in space, the less
massive one doesn't travel
in a perfect circle around the larger one.
«With the majority of Victorian residents
objecting to the $ 300 increase
in their cost of living and
massive inconvenience flowing from the container deposit scheme, it begs the question why are we even considering it?
If an
object is
massive enough, it can actually create detectable gravitational waves, or ripples
in space - time, which scientists saw for the first time earlier this year.
In his framework, the three dimensions of space and time are woven together to create a four - dimensional fabric, which acts as the source of gravity because it bends and warps around
massive objects, like stars.
[1] The ripples
in spacetime known as gravitational waves are created by moving masses, but only the most intense waves, created by rapid speed changes of very
massive objects, can be detected by the current generation of detectors.
Then, effectively by accident, Batygin and Brown noticed that if they ran their simulations with a
massive planet
in an anti-aligned orbit — an orbit
in which the planet's closest approach to the sun, or perihelion, is 180 degrees across from the perihelion of all the other
objects and known planets — the distant Kuiper Belt
objects in the simulation assumed the alignment that is actually observed.
He had solved Einstein's equations of general relativity for the first time, and shown what happens to space - time inside and outside a
massive object —
in this case, a perfectly spherical, non-spinning star.
The
object is located
in the center of a colorful cloud of material consisting of the remains of an ancient star that exploded as a
massive supernova.
Instruments like the 8.4 - meter Large Synoptic Survey Telescope, slated to begin operation
in 2014, will use
massive computer power to carry out continuous scans of sky for near - Earth
objects, leaving ever fewer patches for amateurs to focus on.
«
In a universe with no dark energy, massive objects would just keep growing, which results in more gravitational lensing,» says Sudeep Das of the University of California, Berkele
In a universe with no dark energy,
massive objects would just keep growing, which results
in more gravitational lensing,» says Sudeep Das of the University of California, Berkele
in more gravitational lensing,» says Sudeep Das of the University of California, Berkeley.
This «gravitational lensing» causes the supernova's light to appear brighter and sometimes
in multiple locations, if the light rays travel different paths around the
massive object.
Planet ejections occur as a result of a close planetary encounter
in which one of the
objects accelerates so much that it breaks free from the
massive gravitational pull of the Sun.
All the previous gravitational - wave detections since the first
in September 2015 had been the result of two merging black holes —
objects much more
massive than a neutron star — which have left only gravitational waves as fleeting clues of their merger.
A dense atmosphere like Earth's is relatively rare
in our solar system because an
object has to be sufficiently
massive to have enough gravity to hold onto it.
For the first time, scientists using NASA's Hubble Space Telescope have witnessed a
massive object with the makeup of a comet being ripped apart and scattered
in the atmosphere of a white dwarf, the burned - out remains of a compact star.
Einstein predicted that the movement of
massive objects changing the curvature of space - time should produce waves
in that fabric.
Doing so would make it possible to detect gravitational waves, faint ripples
in space - time that, according to Einstein, emanate from interactions between
massive objects like neutron stars and supermassive black holes.
The team will also make modifications to the telescope's instrumentation, which will allow scientists to look even further back
in time, to before there were enough stars to form galaxies, when the very first population of very
massive objects began to blossom.
If HERA succeeds, this radio telescope array
in South Africa could reveal new information about the slow roast of universal reionization, the identities of the very first
massive objects, the evolution of the cosmic ingredients list and perhaps even clues about the mechanism behind the formation of the first
massive objects.
But soon after astronomers
in the
Massive Compact Halo
Object (MACHO) survey team discovered MACHO -97-BLG on 19 June 1997, they realized the object's flickering was too complex to result from a single - star
Object (MACHO) survey team discovered MACHO -97-BLG on 19 June 1997, they realized the
object's flickering was too complex to result from a single - star
object's flickering was too complex to result from a single - star lens.
Einstein's general theory of relativity predicts that gravitational waves — ripples
in spacetime — emanate from accelerating
massive objects.
The concept of an
object so
massive that not even light can escape the pull of its gravity was first mooted way back
in 1783.
Whereas Newtonian gravity was a mysterious force that somehow emanated from mass and acted instantaneously over long distances,
in Einstein's view a
massive object simply curves the space - time fabric around it.
Doing so would make it possible to detect gravitational waves, faint ripples
in space - time that, according to Einstein, emanate from interactions between
massive objects such as neutron stars and supermassive black holes.
Sometimes that can result
in a faraway
object appearing distorted or even multiple times around a nearer
massive object, like a menu viewed through the bottom of a wine glass.
Minute tremors
in space itself, predicted by Einstein's general theory of relativity, are generated when
massive objects accelerate.
In the early universe, galaxies collided relatively often and their black holes sometimes merged, growing more massive in the process and sometimes birthing hugely energetic objects known as quasar
In the early universe, galaxies collided relatively often and their black holes sometimes merged, growing more
massive in the process and sometimes birthing hugely energetic objects known as quasar
in the process and sometimes birthing hugely energetic
objects known as quasars.
Last April astronomical detectives announced a break: An orbiting X-ray observatory picked up the chemical fingerprints of several elements
in a burst's afterglow, identifying the
object as an unusual type of supernova — the detonation of a
massive, dying star.
Another, much smaller effect is gravitomagnetism, or frame - dragging,
in which the spin of a
massive object tugs space - time
in the direction of its rotation, like a spoon twisted
in honey (see «A twist
in space - time»).
Black holes are
massive objects that have collapsed
in on themselves, creating a gravitational suction so intense that their insides become cut off from the rest of the universe.
There's an intriguing twist, too: Jayawardhana and others have shown that young brown dwarfs generally do not have
massive protoplanetary disks of gas and dust, which means that if the new
object is indeed a planet, it may not have formed the same way planets
in our solar system did.