The most -
studied galaxy in the universe — the Milky Way — might not be as «typical» as previously thought, according to a new study.
Even though the Milky Way is the most
studied galaxy in the universe, there's still so much we don't know about it.
Not exact matches
The discovery is promising for NASA's upcoming James Webb Space Telescope, which will launch
in 2018 on a mission to
study these embryonic
galaxies from the
universe's distant dawn
in much more detail.
One of the oldest known
galaxies in the
universe is now home to the oldest oxygen yet spotted, a new
study suggests.
«Every confirmation adds another piece to the puzzle of how the first generations of
galaxies formed
in the early
universe,» said Pieter van Dokkum, the Sol Goldman Family Professor of Astronomy and chair of Yale's Department of Astronomy, who is second author of the
study.
The reionization of hydrogen
in the
universe didn't occur like the flipping on of a light switch; it wasn't instantaneous and probably didn't happen at the same rate across the cosmos, said Anna Frebel, an assistant professor of physics at MIT who
studies stars and
galaxies that formed
in the very early days of the
universe.
George Becker of the University of Cambridge and colleagues
studied the light coming from
galaxies at different times
in the
universe's history.
«Dust is ubiquitous
in nearby and more distant
galaxies, but has, until recently, been very difficult to detect
in the very early
universe,» says University of Edinburgh astrophysicist Michal Michalowski, who was not involved
in the
study.
«
In contrast to the well - studied galaxies in clusters — the «cities» of the universe — we know relatively little about the properties of galaxies in voids.&raqu
In contrast to the well -
studied galaxies in clusters — the «cities» of the universe — we know relatively little about the properties of galaxies in voids.&raqu
in clusters — the «cities» of the
universe — we know relatively little about the properties of
galaxies in voids.&raqu
in voids.»
In a joint collaboration between the California Institute of Technology and the University of California, Riverside, astronomers have performed an extensive
study of the properties of
galaxies within filaments formed at different times during the age of the
universe.
Many of the Smithsonian's 1000 scientists and research fellows are engaged
in research related to two challenges: understanding the
universe by
studying stars, planets, and
galaxies and understanding and sustaining a biodiverse planet.
For years he had been
studying the origin of the
universe, working backward
in time from the current arrangement of
galaxies to infer conditions
in the era immediately after the Big Bang.
The
study, published online today
in The Astrophysical Journal Letters, describes how the researchers used the powerful MOSFIRE instrument on the W. M. Keck Observatory's 10 - meter telescope
in Hawaii to peer into a time when the
universe was still very young and see what the
galaxy looked like only 670 million years after the big bang.
(I never did, but my undergrad adviser, Martha Haynes, uses Arecibo to
study the distribution of
galaxies in the local
universe.)
«It boggles the mind that over 90 percent of the
galaxies in the
universe have yet to be
studied.
With them it will peer through the creaking, dusty cosmic eons to
study much that astronomers using Hubble and other telescopes have barely begun to glimpse: the
universe's very first
galaxies, nascent stars and planets
in mid-creation
in nebulous wombs, the atmospheres of worlds both within and beyond our solar system.
Webb — custom - built to
study these murky epochs — could use gravitational lensing to unveil these and even older
galaxies in sufficient detail and number to pin down exactly how these ancient objects arose and first brought light into the
universe.
The
study's researchers concluded that at least 10 times more
galaxies exist
in the observable
universe than previously thought.
The main aim of LOFAR is to
study the era
in the early
universe when the very first stars and
galaxies were forming and ionizing all the interstellar gas around them.
By
studying such a large data set — over 200,000
galaxies in 21 different wavelengths, or colors of light, from ultraviolet to infrared — astronomers compared the energy emissions from
galaxies across a wide swath of space and time to read the history of the
universe.
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.
Hence, it is one of the most -
studied starburst
galaxies in the nearby
universe within 500 million light - years of the Sun.
Led by Sandra Savaglio and Karl Glazebrook of Johns Hopkins University
in Baltimore, Maryland, the team
studied a few hundred
galaxies at distances of some 10 billion light - years, looking back to a time when the
universe was only about 4 billion years old.
Astronomers have never been able to
study normal
galaxies in much detail
in this early epoch of the
universe.
A new
study based on observations with the Hubble Space Telescope has shown that the most massive
galaxies in the
universe, which are found
in clusters like this, have been aligned with the distribution of neighboring
galaxies for at least 10 billion years.
In more recent
studies the
universe appears as a collection of giant bubble - like voids separated by sheets and filaments of
galaxies, with the superclusters appearing as occasional relatively dense nodes.
By comparison, the
study by Tremblay and his colleagues looked at only elliptical
galaxies in the nearby
universe with fireworks at their centers.
These events will be dramatic:
In terms of energy, two merging black holes should «outshine every star in every galaxy in the universe in their final moments,» says Montana State's Cornish, who studies how to make sense of the data that will soon pour in from LIGO, Virgo and other gravitational wave experiment
In terms of energy, two merging black holes should «outshine every star
in every galaxy in the universe in their final moments,» says Montana State's Cornish, who studies how to make sense of the data that will soon pour in from LIGO, Virgo and other gravitational wave experiment
in every
galaxy in the universe in their final moments,» says Montana State's Cornish, who studies how to make sense of the data that will soon pour in from LIGO, Virgo and other gravitational wave experiment
in the
universe in their final moments,» says Montana State's Cornish, who studies how to make sense of the data that will soon pour in from LIGO, Virgo and other gravitational wave experiment
in their final moments,» says Montana State's Cornish, who
studies how to make sense of the data that will soon pour
in from LIGO, Virgo and other gravitational wave experiment
in from LIGO, Virgo and other gravitational wave experiments.
A new
study led by University of California, Riverside astronomers casts light on how young, hot stars ionize oxygen
in the early
universe and the effects on the evolution of
galaxies through time.
In a 2013 observational study, University of Wisconsin - Madison astronomer Amy Barger and her then - student Ryan Keenan showed that our galaxy, in the context of the large - scale structure of the universe, resides in an enormous void — a region of space containing far fewer galaxies, stars and planets than expecte
In a 2013 observational
study, University of Wisconsin - Madison astronomer Amy Barger and her then - student Ryan Keenan showed that our
galaxy,
in the context of the large - scale structure of the universe, resides in an enormous void — a region of space containing far fewer galaxies, stars and planets than expecte
in the context of the large - scale structure of the
universe, resides
in an enormous void — a region of space containing far fewer galaxies, stars and planets than expecte
in an enormous void — a region of space containing far fewer
galaxies, stars and planets than expected.
«This ultraluminous quasar with its supermassive black hole provides a unique laboratory to the
study of the mass assembly and
galaxy formation around the most massive black holes
in the early
universe.»
The newly discovered black hole is
in a
galaxy, NGC 1600,
in the opposite part of the sky from the Coma Cluster
in a relative desert, said the leader of the discovery team, Chung - Pei Ma, a UC Berkeley professor of astronomy and head of the MASSIVE Survey, a
study of the most massive
galaxies and black holes
in the local
universe with the goal of understanding how they form and grow supermassive.
The
study pokes holes
in the current understanding of
galaxy formation and questions the accepted model of the origin and evolution of the
universe.
The
galaxy was detected as part of the Frontier Fields program, an ambitious three - year effort, begun
in 2013, that teams Hubble with NASA's other Great Observatories — the Spitzer Space Telescope and the Chandra X-ray Observatory — to probe the early
universe by
studying large
galaxy clusters.
A new
study has come to the startling conclusion that as many as half of all stars
in the
universe may be rogue, having been ejected from their birthplaces by
galaxy collisions or mergers.
Astronomers
studying the motions of
galaxies and the character of the cosmic microwave background radiation came to realize
in the last century that most of the matter
in the
universe was not visible.
g (acceleration due to gravity) G (gravitational constant) G star G1.9 +0.3 gabbro Gabor, Dennis (1900 — 1979) Gabriel's Horn Gacrux (Gamma Crucis) gadolinium Gagarin, Yuri Alexeyevich (1934 — 1968) Gagarin Cosmonaut Training Center GAIA Gaia Hypothesis galactic anticenter galactic bulge galactic center Galactic Club galactic coordinates galactic disk galactic empire galactic equator galactic habitable zone galactic halo galactic magnetic field galactic noise galactic plane galactic rotation galactose Galatea
GALAXIES galaxy galaxy cannibalism
galaxy classification
galaxy formation
galaxy interaction
galaxy merger
Galaxy, The
Galaxy satellite series Gale Crater Galen (c. AD 129 — c. 216) galena GALEX (
Galaxy Evolution Explorer) Galilean satellites Galilean telescope Galileo (Galilei, Galileo)(1564 — 1642) Galileo (spacecraft) Galileo Europa Mission (GEM) Galileo satellite navigation system gall gall bladder Galle, Johann Gottfried (1812 — 1910) gallic acid gallium gallon gallstone Galois, Évariste (1811 — 1832) Galois theory Galton, Francis (1822 — 1911) Galvani, Luigi (1737 — 1798) galvanizing galvanometer game game theory GAMES AND PUZZLES gamete gametophyte Gamma (Soviet orbiting telescope) Gamma Cassiopeiae Gamma Cassiopeiae star gamma function gamma globulin gamma rays Gamma Velorum gamma - ray burst gamma - ray satellites Gamow, George (1904 — 1968) ganglion gangrene Ganswindt, Hermann (1856 — 1934) Ganymede «garbage theory», of the origin of life Gardner, Martin (1914 — 2010) Garneau, Marc (1949 ---RRB- garnet Garnet Star (Mu Cephei) Garnet Star Nebula (IC 1396) garnierite Garriott, Owen K. (1930 ---RRB- Garuda gas gas chromatography gas constant gas giant gas laws gas - bounded nebula gaseous nebula gaseous propellant gaseous - propellant rocket engine gasoline Gaspra (minor planet 951) Gassendi, Pierre (1592 — 1655) gastric juice gastrin gastrocnemius gastroenteritis gastrointestinal tract gastropod gastrulation Gatewood, George D. (1940 ---RRB- Gauer - Henry reflex gauge boson gauge theory gauss (unit) Gauss, Carl Friedrich (1777 — 1855) Gaussian distribution Gay - Lussac, Joseph Louis (1778 — 1850) GCOM (Global Change Observing Mission) Geber (c. 720 — 815) gegenschein Geiger, Hans Wilhelm (1882 — 1945) Geiger - Müller counter Giessler tube gel gelatin Gelfond's theorem Gell - Mann, Murray (1929 ---RRB- GEM «gemination,» of martian canals Geminga Gemini (constellation) Gemini Observatory Gemini Project Gemini - Titan II gemstone gene gene expression gene mapping gene pool gene therapy gene transfer General Catalogue of Variable Stars (GCVS) general precession general theory of relativity generation ship generator Genesis (inflatable orbiting module) Genesis (sample return probe) genetic code genetic counseling genetic disorder genetic drift genetic engineering genetic marker genetic material genetic pool genetic recombination genetics GENETICS AND HEREDITY Geneva Extrasolar Planet Search Program genome genome, interstellar transmission of genotype gentian violet genus geoboard geode geodesic geodesy geodesy satellites geodetic precession Geographos (minor planet 1620) geography GEOGRAPHY Geo - IK geologic time geology GEOLOGY AND PLANETARY SCIENCE geomagnetic field geomagnetic storm geometric mean geometric sequence geometry GEOMETRY geometry puzzles geophysics GEOS (Geodetic Earth Orbiting Satellite) Geosat geostationary orbit geosynchronous orbit geosynchronous / geostationary transfer orbit (GTO) geosyncline Geotail (satellite) geotropism germ germ cells Germain, Sophie (1776 — 1831) German Rocket Society germanium germination Gesner, Konrad von (1516 — 1565) gestation Get Off the Earth puzzle Gettier problem geyser g - force GFO (Geosat Follow - On) GFZ - 1 (GeoForschungsZentrum) ghost crater Ghost Head Nebula (NGC 2080) ghost image Ghost of Jupiter (NGC 3242) Giacconi, Riccardo (1931 ---RRB- Giacobini - Zinner, Comet (Comet 21P /) Giaever, Ivar (1929 ---RRB- giant branch Giant Magellan Telescope giant molecular cloud giant planet giant star Giant's Causeway Giauque, William Francis (1895 — 1982) gibberellins Gibbs, Josiah Willard (1839 — 1903) Gibbs free energy Gibson, Edward G. (1936 ---RRB- Gilbert, William (1544 — 1603) gilbert (unit) Gilbreath's conjecture gilding gill gill (unit) Gilruth, Robert R. (1913 — 2000) gilsonite gimbal Ginga ginkgo Giotto (ESA Halley probe) GIRD (Gruppa Isutcheniya Reaktivnovo Dvisheniya) girder glacial drift glacial groove glacier gland Glaser, Donald Arthur (1926 — 2013) Glashow, Sheldon (1932 ---RRB- glass GLAST (Gamma - ray Large Area Space Telescope) Glauber, Johann Rudolf (1607 — 1670) glaucoma glauconite Glenn, John Herschel, Jr. (1921 ---RRB- Glenn Research Center Glennan, T (homas) Keith (1905 — 1995) glenoid cavity glia glial cell glider Gliese 229B Gliese 581 Gliese 67 (HD 10307, HIP 7918) Gliese 710 (HD 168442, HIP 89825) Gliese 86 Gliese 876 Gliese Catalogue glioma glissette glitch Global Astrometric Interferometer for Astrophysics (GAIA) Global Oscillation Network Group (GONG) Globalstar globe Globigerina globular cluster globular proteins globule globulin globus pallidus GLOMR (Global Low Orbiting Message Relay) GLONASS (Global Navigation Satellite System) glossopharyngeal nerve Gloster E. 28/39 glottis glow - worm glucagon glucocorticoid glucose glucoside gluon Glushko, Valentin Petrovitch (1908 — 1989) glutamic acid glutamine gluten gluteus maximus glycerol glycine glycogen glycol glycolysis glycoprotein glycosidic bond glycosuria glyoxysome GMS (Geosynchronous Meteorological Satellite) GMT (Greenwich Mean Time) Gnathostomata gneiss Go Go, No - go goblet cell GOCE (Gravity field and steady - state Ocean Circulation Explorer) God Goddard, Robert Hutchings (1882 — 1945) Goddard Institute for Space
Studies Goddard Space Flight Center Gödel, Kurt (1906 — 1978) Gödel
universe Godwin, Francis (1562 — 1633) GOES (Geostationary Operational Environmental Satellite) goethite goiter gold Gold, Thomas (1920 — 2004) Goldbach conjecture golden ratio (phi) Goldin, Daniel Saul (1940 ---RRB- gold - leaf electroscope Goldstone Tracking Facility Golgi, Camillo (1844 — 1926) Golgi apparatus Golomb, Solomon W. (1932 — 2016) golygon GOMS (Geostationary Operational Meteorological Satellite) gonad gonadotrophin - releasing hormone gonadotrophins Gondwanaland Gonets goniatite goniometer gonorrhea Goodricke, John (1764 — 1786) googol Gordian Knot Gordon, Richard Francis, Jr. (1929 — 2017) Gore, John Ellard (1845 — 1910) gorge gorilla Gorizont Gott loop Goudsmit, Samuel Abraham (1902 — 1978) Gould, Benjamin Apthorp (1824 — 1896) Gould, Stephen Jay (1941 — 2002) Gould Belt gout governor GPS (Global Positioning System) Graaf, Regnier de (1641 — 1673) Graafian follicle GRAB graben GRACE (Gravity Recovery and Climate Experiment) graceful graph gradient Graham, Ronald (1935 ---RRB- Graham, Thomas (1805 — 1869) Graham's law of diffusion Graham's number GRAIL (Gravity Recovery and Interior Laboratory) grain (cereal) grain (unit) gram gram - atom Gramme, Zénobe Théophile (1826 — 1901) gramophone Gram's stain Gran Telescopio Canarias (GTC) Granat Grand Tour grand unified theory (GUT) Grandfather Paradox Granit, Ragnar Arthur (1900 — 1991) granite granulation granule granulocyte graph graph theory graphene graphite GRAPHS AND GRAPH THEORY graptolite grass grassland gravel graveyard orbit gravimeter gravimetric analysis Gravitational Biology Facility gravitational collapse gravitational constant (G) gravitational instability gravitational lens gravitational life gravitational lock gravitational microlensing GRAVITATIONAL PHYSICS gravitational slingshot effect gravitational waves graviton gravity gravity gradient gravity gradient stabilization Gravity Probe A Gravity Probe B gravity - assist gray (Gy) gray goo gray matter grazing - incidence telescope Great Annihilator Great Attractor great circle Great Comets Great Hercules Cluster (M13, NGC 6205) Great Monad Great Observatories Great Red Spot Great Rift (
in Milky Way) Great Rift Valley Great Square of Pegasus Great Wall greater omentum greatest elongation Green, George (1793 — 1841) Green, Nathaniel E. Green, Thomas Hill (1836 — 1882) green algae Green Bank Green Bank conference (1961) Green Bank Telescope green flash greenhouse effect greenhouse gases Green's theorem Greg, Percy (1836 — 1889) Gregorian calendar Grelling's paradox Griffith, George (1857 — 1906) Griffith Observatory Grignard, François Auguste Victor (1871 — 1935) Grignard reagent grike Grimaldi, Francesco Maria (1618 — 1663) Grissom, Virgil (1926 — 1967) grit gritstone Groom Lake Groombridge 34 Groombridge Catalogue gross ground, electrical ground state ground - track group group theory GROUPS AND GROUP THEORY growing season growth growth hormone growth hormone - releasing hormone growth plate Grudge, Project Gruithuisen, Franz von Paula (1774 — 1852) Grus (constellation) Grus Quartet (NGC 7552, NGC 7582, NGC 7590, and NGC 7599) GSLV (Geosynchronous Satellite Launch Vehicle) g - suit G - type asteroid Guericke, Otto von (1602 — 1686) guanine Guiana Space Centre guidance, inertial Guide Star Catalog (GSC) guided missile guided missiles, postwar development Guillaume, Charles Édouard (1861 — 1938) Gulf Stream (ocean current) Gulfstream (jet plane) Gullstrand, Allvar (1862 — 1930) gum Gum Nebula gun metal gunpowder Gurwin Gusev Crater gut Gutenberg, Johann (c. 1400 — 1468) Guy, Richard Kenneth (1916 ---RRB- guyot Guzman Prize gymnosperm gynecology gynoecium gypsum gyrocompass gyrofrequency gyropilot gyroscope gyrostabilizer Gyulbudagian's Nebula (HH215)
It records the spectra of up to 50 objects simultaneously, especially useful for
studies of
galaxies in the most distant reaches, and earliest times, of the
universe.
The survey's researchers analyzed light from 26 million
galaxies to
study how structures
in the
universe have changed over the past 7 billion years — half the age of the
universe.
LRIS also records the spectra of up to 50 objects simultaneously, especially useful for
studies of clusters of
galaxies in the most distant reaches, and earliest times, of the
universe.
The technology, known as Laser Guide Star adaptive optics, will lead to important advances
in the
study of planets both inside and outside our solar system, as well as of
galaxies, black holes, and how the
universe formed and evolved, Ghez said.
A
study released Wednesday shows that the first
galaxies in the early
universe may have been the catalyst behind cosmic reionization.
The
study used data from the Baryon Oscillation Spectroscopic Survey, or BOSS, an Earth - based sky survey that captured light from about 1.5 million
galaxies to
study the
universe's expansion and the patterned distribution of matter
in the
universe set
in motion by the propagation of sound waves, or «baryonic acoustic oscillations,» rippling
in the early
universe.
By
studying the statistical properties of the shapes of very distant
galaxies and quasars, astronomers can use the effects of weak lensing to
study the distribution of dark matter
in the
universe.
«Star - formation
studies of this
galaxy provide a stepping stone to understand star formation
in the early
universe.»
The GBT will be used to
study everything from the formation of
galaxies in the early
universe, to the chemical make - up of the dust and gas inside
galaxies and
in the voids that separate them, to the birth processes of stars.
But,
in the early
universe, their
study shows that the 3C 298
galaxy is 100 times less massive than it should be given its behemoth supermassive black hole mass.
«Every confirmation adds another piece to the puzzle of how the first generations of
galaxies formed
in the early
universe,» said Pieter van Dokkum of the Yale University, second author of the
study.
«Although the
galaxy is not as youthful as was once believed, it is certainly developmentally challenged and unique
in the nearby
universe,» said astronomer Alessandra Aloisi from the Space Telescope Science Institute and the European Space Agency
in Baltimore, Md., who led the new
study.
The goal of the survey is to
study the stellar, gaseous, and blackhole content of
galaxies at this important era
in the history of the
universe.