To gauge 3C 58's distance, astronomers exploit the Milky Way's rotation, measuring velocities
of hydrogen clouds in front of the nebula to deduce how fast it revolves around the galaxy's center.
Astrophysicists simulated the fate
of a hydrogen cloud as massive as 10,000 suns that suddenly wafted near a black hole.
Not exact matches
The emergence
of chemistry had a transformative effect on the universe because
of a peculiar property
of atomic
hydrogen: If you take a big
cloud of hydrogen atoms and let it collapse, it gets hotter and hotter until all the bound - up energy keeps it from shrinking any further.
We suspect that water, the constituent
of Saturn's deepest
cloud deck, can suppress convection in the lighter
hydrogen atmosphere for a period
of decades, until finally buoyancy wins out and a large convective outburst ensues.
He says this might be the most interesting epoch
of all — a time when the primordial clumps
of hydrogen took shape, becoming the
clouds from which the first stars and galaxies would eventually form.
Clumpiness begot more clumpiness, as gravity pulled more matter into these dense regions, and
clouds of gas, composed mostly
of hydrogen atoms, began to assemble.
Hydrogen molecules aren't the best coolant, but they are good enough to enable giant gas
clouds, millions
of times as massive as the sun, to fall in on themselves.
Perhaps they were born «obese», forming when vast
clouds of atomic
hydrogen collapsed.
A molecular
cloud is an interstellar
cloud of dust, gas, and a variety
of molecules ranging from molecular
hydrogen (H2) to complex, carbon - containing organics.
Within these
clouds, on the surfaces
of tiny dust grains,
hydrogen atoms link with oxygen to form water.
Young star clusters and
clouds of hydrogen that formed in our galaxy help trace the shapes
of the Milky Way's arms, so astronomers are reasonably certain that it has a spiral structure (see right).
In 2008, a
cloud of hydrogen with a mass then estimated at about 1 million suns was found to be colliding with our galaxy.
Out
of the primordial
hydrogen and helium created in the Big Bang,
clouds coalesced within 100 million years, eventually forming the first stars.
Stars emerge when
clouds of hydrogen molecules coalesce under their collective gravitational attraction.
H II regions like RCW 106 are
clouds of hydrogen gas that are being ionised by the intense starlight
of scorching - hot, young stars, causing them to glow and display weird and wonderful shapes.
Far beyond the pair, immense dusty
hydrogen clouds form an obscuring backdrop, while Scorpius's leftmost edge marks the direction to the turbulent center
of our galaxy.
Complex organic molecules, consisting
of carbon bonded with other elements like oxygen and
hydrogen, are common in the Milky Way, but it was uncertain whether they would be produced in certain dwarf galaxies like the neighboring Large Magellanic
Cloud.
He doubts that an Earth - like planet or super-Earth would pull in so much
hydrogen from the
cloud of gas surrounding a young star.
Most SETI projects tune in to the 1.42 to 1.72 - gigahertz range, reasoning that alien astronomers might expect earthly scientists to be looking there anyway as this is the frequency
of radiation emitted by interstellar
hydrogen and hydroxyl
clouds.
The diffuse
cloud in this image, taken with the Carnegie Institution for Science's Swope telescope in Chile, is the shell
of hot
hydrogen gas ejected by a white dwarf star on March 11, 1437.
Cloud formations made
of ammonia, hydrocarbons and water swirl in a frigid soup
of hydrogen and helium.
Hallis previously used
hydrogen isotope ratios in volcanic basalt rocks to conclude that Earth's water may in fact have been part
of the very dust
cloud from which the planet first condensed.
About 4.6 billion years ago, an enormous
cloud of hydrogen gas and dust collapsed under its own weight, eventually flattening into a disk called the solar nebula.
Now, Christopher Howk and Nicolas Lehner
of the University
of Notre Dame in Indiana have detected fast - moving
clouds of ionised
hydrogen in our galaxy.
At the time our solar system formed about 4.6 billion years ago, only about 39 %
of the
hydrogen and helium in our galaxy had collapsed into
clouds that then evolved into stars, they say.
When they grew to about 10 times the mass
of Earth, their gravity pulled in gas from their birth
cloud, giving them thick atmospheres made mainly
of hydrogen around their solid cores.
If they are
clouds, they're probably made
of ethane, acetylene or
hydrogen cyanide, based on what researchers have learned about Pluto's atmosphere — though they might not be
clouds, just reflective splotches on
«Immense
cloud of hydrogen discovered escaping from exoplanet the size
of Neptune.»
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.
The expanding shock front will heat and stir up the material
of the Galaxy as it spreads outward, encouraging the mixing
of heavy elements made inside stars with
clouds of hydrogen gas in interstellar space, and influencing the evolution
of the Galaxy as a whole.
In the spectrum, the team found evidence
of a large concentration
of neutral
hydrogen clouds close to the galaxy, indicating the presence
of a giant cluster
of embryonic galaxies.
In addition to ash, the eruptive
cloud consisted primarily
of vast quantities
of sulfur dioxide (SO2),
hydrogen chloride (HCl), and
hydrogen fluoride gases (HF).
If
clouds of hydrogen also cluster around quasars — which convert all nearby neutral
hydrogen to invisible ionized gas — then quasars must have ionized more
hydrogen than astronomers had assumed, Savaglio says.
Now images taken by the Hubble Space Telescope have revealed a large
cloud of hydrogen and oxygen — most likely in the form
of water vapour — extending from the moon's south pole.
The images
of infrared light coming from glowing
hydrogen show that the
cloud was compact both before and after its closest approach, as it swung around the black hole.
Instead
of searching for the light from individual galaxies with an optical telescope, the team stalked a different quarry, red - shifted radio waves emitted by
hydrogen atoms floating in huge
clouds within the galaxies.
Since stars are born when dense
clouds of hydrogen molecules collapse, the rate
of star formation and the availability
of molecular
hydrogen, the fuel for star formation, are inextricably linked.
The
cloud consists
of ionized gas, or plasma, and contains the elements
hydrogen, helium, and oxygen, along with heavier elements that were generated during the blast itself.
These fields will do double duty: They will heat a
cloud of hydrogen to the searing temperature required for fusion while forcing the resulting plasma to sit in a ring - shaped
cloud away from the tokamak's walls.
We know that about 4.6 billion years ago, in an outer spiral arm
of the Milky Way, a dense
cloud of hydrogen gas and dust began to collapse in on itself.
Its source appears to be a glowing
cloud of warm molecular
hydrogen, in the spiral galaxy Messier 83.
The mane is a
cloud of cold gas, mostly
hydrogen, that is fluorescing.
The sharp detail
of the spiral's arms, defined by dark, dusty areas and bright, pink
clouds of hydrogen, impressed the judges.
The California Nebula, named for its resemblance to the state, is the
cloud of glowing red
hydrogen gas at left.
The contrasting faint reddish
clouds that seem to weave between the stars are composed
of ionised
hydrogen gas.
If so, astronomers could hunt for them by detecting gamma rays, neutrinos, and even antimatter radiating from interstellar and intergalactic
clouds of hydrogen gas.
He and his colleagues slammed a beam
of heavy
hydrogen atoms into a
cloud composed
of more heavy
hydrogen.
The researchers detected molecules
of carbon monoxide and two forms
of hydrogen in the
clouds, they report today in Astronomy & Astrophysics.
At the center
of the
cloud, matter would pile up to densities and temperatures that (scientists later realized) were high enough to allow
hydrogen atoms to fuse into helium.
They found a large
cloud of hydrogen and oxygen extending from the moon's south pole.