- published: 10 Sep 2015
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Stellar mass is a phrase that is used by astronomers to describe the mass of a star. It is usually enumerated in terms of the Sun's mass as a proportion of a solar mass (M☉). Hence, the bright star Sirius has around 2.02 M☉. A star's mass will vary over its lifetime as additional mass becomes accreted, such as from a companion star, or mass is ejected with the stellar wind or pulsational behavior.
Stars are sometimes grouped by mass based upon their evolutionary behavior as they approach the end of their nuclear fusion lifetimes. Very low mass stars with masses below 0.5 M☉ do not enter the asymptotic giant branch (AGB) but evolve directly into white dwarfs. Low mass stars with a mass below about 1.8–2.2 M☉ (depending on composition) do enter the AGB, where they develop a degenerate helium core. Intermediate-mass stars undergo helium fusion and develop a degenerate carbon-oxygen core. Massive stars have a minimum mass of 7–10 M☉, but this may be as low as 5–6 M☉. These stars undergo carbon fusion, with their lives ending in a core-collapse supernova explosion.Black holes created as a result of a stellar collapse are termed stellar mass black holes.
Crash Course (also known as Driving Academy) is a 1988 made for television teen film directed by Oz Scott.
Crash Course centers on a group of high schoolers in a driver’s education class; many for the second or third time. The recently divorced teacher, super-passive Larry Pearl, is on thin ice with the football fanatic principal, Principal Paulson, who is being pressured by the district superintendent to raise driver’s education completion rates or lose his coveted football program. With this in mind, Principal Paulson and his assistant, with a secret desire for his job, Abner Frasier, hire an outside driver’s education instructor with a very tough reputation, Edna Savage, aka E.W. Savage, who quickly takes control of the class.
The plot focuses mostly on the students and their interactions with their teachers and each other. In the beginning, Rico is the loner with just a few friends, Chadley is the bookish nerd with few friends who longs to be cool and also longs to be a part of Vanessa’s life who is the young, friendly and attractive girl who had to fake her mother’s signature on her driver’s education permission slip. Kichi is the hip-hop Asian kid who often raps what he has to say and constantly flirts with Maria, the rich foreign girl who thinks that the right-of-way on the roadways always goes to (insert awesomely fake foreign Latino accent) “my father’s limo”. Finally you have stereotypical football meathead J.J., who needs to pass his English exam to keep his eligibility and constantly asks out and gets rejected by Alice, the tomboy whose father owns “Santini & Son” Concrete Company. Alice is portrayed as being the “son” her father wanted.
Spaceflight (also written space flight) is ballistic flight into or through outer space. Spaceflight can occur with spacecraft with or without humans on board. Examples of human spaceflight include the U.S. Apollo Moon landing and Space Shuttle programs and the Russian Soyuz program, as well as the ongoing International Space Station. Examples of unmanned spaceflight include space probes that leave Earth orbit, as well as satellites in orbit around Earth, such as communications satellites. These operate either by telerobotic control or are fully autonomous.
Spaceflight is used in space exploration, and also in commercial activities like space tourism and satellite telecommunications. Additional non-commercial uses of spaceflight include space observatories, reconnaissance satellites and other Earth observation satellites.
A spaceflight typically begins with a rocket launch, which provides the initial thrust to overcome the force of gravity and propels the spacecraft from the surface of the Earth. Once in space, the motion of a spacecraft—both when unpropelled and when under propulsion—is covered by the area of study called astrodynamics. Some spacecraft remain in space indefinitely, some disintegrate during atmospheric reentry, and others reach a planetary or lunar surface for landing or impact.
A hole is an opening.
Hole or holes may also refer to:
The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory established on May 1, 1959 as NASA's first space flight center. GSFC employs approximately 10,000 civil servants and contractors, and is located approximately 6.5 miles (10.5 km) northeast of Washington, D.C. in Greenbelt, Maryland, USA. GSFC, one of ten major NASA field centers, is named in recognition of Dr. Robert H. Goddard (1882–1945), the pioneer of modern rocket propulsion in the United States.
GSFC is the largest combined organization of scientists and engineers in the United States dedicated to increasing knowledge of the Earth, the Solar System, and the Universe via observations from space. GSFC is a major U.S. laboratory for developing and operating unmanned scientific spacecraft. GSFC conducts scientific investigation, development and operation of space systems, and development of related technologies. Goddard scientists can develop and support a mission, and Goddard engineers and technicians can design and build the spacecraft for that mission. Goddard scientist John C. Mather shared the 2006 Nobel Prize in Physics for his work on COBE.
Massive stars fuse heavier elements in their cores than lower mass stars. This leads to the creation of heavier elements up to iron. Iron robs critical energy from the core, causing it to collapse. The shock wave, together with a huge swarm of neutrinos, blast through the star’s outer layers, causing it to explode. The resulting supernova creates even more heavy elements, scattering them through space. Also, happily, we’re in no danger from a nearby supernova. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Massive Stars Fuse Heavier Elements Up To Iron 1:15 Iron Uses High Amounts of Energy, Thus Making Stars Collapse 3:58 The Resulting Supernova Creates Even Heavier Elements 10:00 Relax, Something Else Will Kill You 9:04 ...
Today we are talking about the life -- and death -- of stars. Low mass stars live a long time, fusing all their hydrogen into helium over a trillion years. More massive stars like the Sun live shorter lives. They fuse hydrogen into helium, and eventually helium into carbon (and also some oxygen and neon). When this happens they expand, get brighter, and cool off, becoming red giants. They lose most of their mass, exposing their cores, and then cool off over many billions of years. Crash Course Astronomy posters now available at DFTBA: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Low Mass Stars Live a Long Time 0:57 Larger Stars (Like Our Sun) Live Shorter Lives 3:10 Fueled By Fusion 3:58 How They Turn Into Red Giants 5:45 -- PBS Digital Studios: ht...
Music: "Lost in Space" by Lars Leonhard, courtesy of artist. http://www.lars-leonhard.de/ This animation of supercomputer data takes you to the inner zone of the accretion disk of a stellar-mass black hole. Gas heated to 20 million degrees F as it spirals toward the black hole glows in low-energy, or soft, X-rays. Just before the gas plunges to the center, its orbital motion is approaching the speed of light. X-rays up to hundreds of times more powerful ("harder") than those in the disk arise from the corona, a region of tenuous and much hotter gas around the disk. Coronal temperatures reach billions of degrees. The event horizon is the boundary where all trajectories, including those of light, must go inward. Nothing, not even light, can pass outward across the event horizon and escape ...
When massive suns run out of fuel and collapse a stellar black hole forms. It has the power to crush objects the size of the Sun into a 75 mile wide object. Astronomers are studying how these black holes produce their highest-energy light.
How do we figure out how massive a star is if it lives lightyears away from us? Why is the Moon Shrinking? ►►►► http://dne.ws/1PkfHgO DNews Live Tickets Here ►►►► http://dne.ws/1Fa2OCh Read More: Mass of Stars http://www.universetoday.com/25328/mass-of-stars/ “Stars can range in mass from the least massive red dwarf stars to the monstrous hypergiant stars. Let’s take a look at the mass of stars at various sizes.” New Way to Weigh a Star http://www.sciencedaily.com/releases/2015/10/151005082537.htm “Researchers have developed a new method for measuring the mass of pulsars - highly magnetized rotating neutron stars formed from the remains of massive stars after they explode into supernovae.” ____________________ DNews is dedicated to satisfying your curiosity and...
Astronomers using ESOs Very Large Telescope (VLT) have detected a stellar-mass black hole much further away than any other previously known. With a mass twenty times that of the Sun, this is also the second most massive stellar mass black hole ever found. The newly announced black hole lies in a spiral galaxy called NGC 300, six million light-years from Earth. This video zooms in onto the position of the system containing the stellar-mass black hole, and finishes with an artists impression of the system. Credit: ESO/Digitized Sky Survey 2/P. Crowther/L. Calçada This video is available for download in different formats on: http://www.eso.org/public/videos/eso1004b/
We’ve covered a lot of incredible stuff, but this week we’re talking about the weirdest objects in space: BLACK HOLES. Stellar mass black holes form when a very massive star dies, and its core collapses. The core has to be more than about 2.8 times the Sun’s mass to form a black hole. Black holes come in different sizes, but for all of them, the escape velocity is greater than the speed of light, so nothing can escape, not matter or light. They don’t wander the Universe gobbling everything down around them; their gravity is only really intense very close to them. Tides near a stellar mass black hole will spaghettify you, and time slows down when you get near a black hole — not that this helps much if you’re falling in. Crash Course Astronomy Poster: http://store.dftba.com/products/crashco...
INSIDE A BLACK HOLE! Stellar-mass Black Hole Simulation from NASA From NASA: "Peer into a Simulated Stellar-mass Black Hole - This animation of supercomputer data takes you to the inner zone of the accretion disk of a stellar-mass black hole. Gas heated to 20 million degrees Fahrenheit as it spirals toward the black hole glows in low-energy, or soft, X-rays. Just before the gas plunges to the center, its orbital motion is approaching the speed of light. X-rays up to hundreds of times more powerful ('harder') than those in the disk arise from the corona, a region of tenuous and much hotter gas around the disk. Coronal temperatures reach billions of degrees. The event horizon is the boundary where all trajectories, including those of light, must go inward. Nothing, not even light, can pass...
Lowerground Intro Animation. A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star. www.lowerground.com Audio by Michael Fakesch www.michaelfakesch.com
This animation shows the unique triple-star system with a superdense neutron star and two white dwarf stars. The neutron star is a pulsar, emitting lighthouse-like beams of radiation as it spins on its axis. These beams, in blue, are seen sweeping through space as the neutron star rotates. At the start, you see this pulsar and its close companion white dwarf in orbit around their common center of mass. The animation zooms outward, showing this pair also in orbit with a more-distant, cooler white dwarf, and illustrates the motions of these three bodies. The entire system would fit within Earth's orbit around the Sun.
ESO/Digitized Sky Survey 2/P. Crowther/L. Calçada
This artist’s impression shows a stellar flare on star HD 189733A, the parent star of exoplanet HD 189733b. In this video, the surface of the star, which is around 80% the mass of the Sun, is animated based on observations of the Sun from the Solar Dynamics Observatory. Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory More information and download-options: http://www.spacetelescope.org/videos/heic1209f/
a starship flies within tens of thousand of kilometres from a K-class star of about 0.75 the mass of our own sun
CYGNUS is one of the rare conceptual light performances staged in Istanbul to date. Four teams, Bİ'ŞEYLER New Media Works, OUCHHH, Panpiper and Staras came together and set out to explore constellation Cygnus, the Swan, which is home to Cygnus X-1, a galactic X-ray source believed to be a stellar mass black hole. The light installation was performed in a 2400-m2 venue on December 18-19, 2014 in Istanbul. Using 46 Clay Paky Sharpies and 2 Atmosphere Hazers, the performance immersed 2000 viewers in the experience of the constellation which is believed to be about 5 million years old. Light sources were placed to surround the audience at different heights to allow light flow above their heads, creating a void at the center which prompted viewers to interpret the notion of a black hole. ...
In this animation, exoplanet HD 189733b is seen in closeup as it passes in front of its parent star. Hubble observed the planet do this in 2010 and 2011. This simulation depicts the 2011 observations, in which the planet’s atmosphere is evaporating away, possibly under the influence of a stellar flare. In this video, the surface of the star, which is around 80% the mass of the Sun, is animated based on observations of the Sun from the Solar Dynamics Observatory. Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory More information and download-options: http://www.spacetelescope.org/videos/heic1209c/
CROWDFUNDING NOW RUNNING: http://theriseofthesynths.com/crowdfunding The Rise of the Synths is a documentary about the Synthwave scene, nostalgia and the universe of creating sounds. 'The old soundtrack of a new generation' The film is a time travel towards the roots of a worldwide grass-root music scene known as Synthwave, an irresistible blending of modern electronic composition with 80s pop culture’s nostalgia, that over the last two years has transformed from a whisper on selected internet hubs, to a ever-growing scene expanding rapidly as we speak. Accounting millions of plays on social media, devoted fans are legion, but nobody in the mass media knows about them. A time travel into the universe of creating sounds. A love letter to human fascination and the collective memories of...
music by Lucas Thanos images by various artists Black and White Holes A black hole is a mathematically defined region of spacetime exhibiting such a strong gravitational pull that no particle or electromagnetic radiation can escape from it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which no escape is possible is called the event horizon. Although crossing the event horizon has enormous effect on the fate of the object crossing it, it appears to have no locally detectable features. In many ways a black hole acts like an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spec...
CROWDFUNDING NOW RUNNING: http://theriseofthesynths.com/crowdfunding Featuring: Electric Youth, College, Miami Nights 1984, Stellar Dreams, Dance with the dead, Power Glove, Nightcrawler Music, Vincenzo Salvia, Com Truise, The Midnight, Maethelvin, Jordan F, Betamaxx, Futurecop!, Dynatron, Lazerhawk, mitch murder, Darkest, OGRE, Kristine, Carpenter Brut, Timecop1983, Waveshaper, MPM Soundtracks. "A genius is a fool, until his idea succeeds..." You can make this dream come true. The Rise of the Synths is a documentary (and a time travel) about the SynthWave scene. 'The old sountrack of a new generation' The film is a time travel towards the roots of a worldwide grass-root music scene known as Synthwave, an irresistible blending of modern electronic composition with 80s pop culture’s n...
Massive stars fuse heavier elements in their cores than lower mass stars. This leads to the creation of heavier elements up to iron. Iron robs critical energy from the core, causing it to collapse. The shock wave, together with a huge swarm of neutrinos, blast through the star’s outer layers, causing it to explode. The resulting supernova creates even more heavy elements, scattering them through space. Also, happily, we’re in no danger from a nearby supernova. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Massive Stars Fuse Heavier Elements Up To Iron 1:15 Iron Uses High Amounts of Energy, Thus Making Stars Collapse 3:58 The Resulting Supernova Creates Even Heavier Elements 10:00 Relax, Something Else Will Kill You 9:04 ...
Today we are talking about the life -- and death -- of stars. Low mass stars live a long time, fusing all their hydrogen into helium over a trillion years. More massive stars like the Sun live shorter lives. They fuse hydrogen into helium, and eventually helium into carbon (and also some oxygen and neon). When this happens they expand, get brighter, and cool off, becoming red giants. They lose most of their mass, exposing their cores, and then cool off over many billions of years. Crash Course Astronomy posters now available at DFTBA: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Low Mass Stars Live a Long Time 0:57 Larger Stars (Like Our Sun) Live Shorter Lives 3:10 Fueled By Fusion 3:58 How They Turn Into Red Giants 5:45 -- PBS Digital Studios: ht...
Music: "Lost in Space" by Lars Leonhard, courtesy of artist. http://www.lars-leonhard.de/ This animation of supercomputer data takes you to the inner zone of the accretion disk of a stellar-mass black hole. Gas heated to 20 million degrees F as it spirals toward the black hole glows in low-energy, or soft, X-rays. Just before the gas plunges to the center, its orbital motion is approaching the speed of light. X-rays up to hundreds of times more powerful ("harder") than those in the disk arise from the corona, a region of tenuous and much hotter gas around the disk. Coronal temperatures reach billions of degrees. The event horizon is the boundary where all trajectories, including those of light, must go inward. Nothing, not even light, can pass outward across the event horizon and escape ...
When massive suns run out of fuel and collapse a stellar black hole forms. It has the power to crush objects the size of the Sun into a 75 mile wide object. Astronomers are studying how these black holes produce their highest-energy light.
How do we figure out how massive a star is if it lives lightyears away from us? Why is the Moon Shrinking? ►►►► http://dne.ws/1PkfHgO DNews Live Tickets Here ►►►► http://dne.ws/1Fa2OCh Read More: Mass of Stars http://www.universetoday.com/25328/mass-of-stars/ “Stars can range in mass from the least massive red dwarf stars to the monstrous hypergiant stars. Let’s take a look at the mass of stars at various sizes.” New Way to Weigh a Star http://www.sciencedaily.com/releases/2015/10/151005082537.htm “Researchers have developed a new method for measuring the mass of pulsars - highly magnetized rotating neutron stars formed from the remains of massive stars after they explode into supernovae.” ____________________ DNews is dedicated to satisfying your curiosity and...
Astronomers using ESOs Very Large Telescope (VLT) have detected a stellar-mass black hole much further away than any other previously known. With a mass twenty times that of the Sun, this is also the second most massive stellar mass black hole ever found. The newly announced black hole lies in a spiral galaxy called NGC 300, six million light-years from Earth. This video zooms in onto the position of the system containing the stellar-mass black hole, and finishes with an artists impression of the system. Credit: ESO/Digitized Sky Survey 2/P. Crowther/L. Calçada This video is available for download in different formats on: http://www.eso.org/public/videos/eso1004b/
We’ve covered a lot of incredible stuff, but this week we’re talking about the weirdest objects in space: BLACK HOLES. Stellar mass black holes form when a very massive star dies, and its core collapses. The core has to be more than about 2.8 times the Sun’s mass to form a black hole. Black holes come in different sizes, but for all of them, the escape velocity is greater than the speed of light, so nothing can escape, not matter or light. They don’t wander the Universe gobbling everything down around them; their gravity is only really intense very close to them. Tides near a stellar mass black hole will spaghettify you, and time slows down when you get near a black hole — not that this helps much if you’re falling in. Crash Course Astronomy Poster: http://store.dftba.com/products/crashco...
INSIDE A BLACK HOLE! Stellar-mass Black Hole Simulation from NASA From NASA: "Peer into a Simulated Stellar-mass Black Hole - This animation of supercomputer data takes you to the inner zone of the accretion disk of a stellar-mass black hole. Gas heated to 20 million degrees Fahrenheit as it spirals toward the black hole glows in low-energy, or soft, X-rays. Just before the gas plunges to the center, its orbital motion is approaching the speed of light. X-rays up to hundreds of times more powerful ('harder') than those in the disk arise from the corona, a region of tenuous and much hotter gas around the disk. Coronal temperatures reach billions of degrees. The event horizon is the boundary where all trajectories, including those of light, must go inward. Nothing, not even light, can pass...
Lowerground Intro Animation. A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star. www.lowerground.com Audio by Michael Fakesch www.michaelfakesch.com
This animation shows the unique triple-star system with a superdense neutron star and two white dwarf stars. The neutron star is a pulsar, emitting lighthouse-like beams of radiation as it spins on its axis. These beams, in blue, are seen sweeping through space as the neutron star rotates. At the start, you see this pulsar and its close companion white dwarf in orbit around their common center of mass. The animation zooms outward, showing this pair also in orbit with a more-distant, cooler white dwarf, and illustrates the motions of these three bodies. The entire system would fit within Earth's orbit around the Sun.
ESO/Digitized Sky Survey 2/P. Crowther/L. Calçada
This artist’s impression shows a stellar flare on star HD 189733A, the parent star of exoplanet HD 189733b. In this video, the surface of the star, which is around 80% the mass of the Sun, is animated based on observations of the Sun from the Solar Dynamics Observatory. Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory More information and download-options: http://www.spacetelescope.org/videos/heic1209f/
a starship flies within tens of thousand of kilometres from a K-class star of about 0.75 the mass of our own sun
CYGNUS is one of the rare conceptual light performances staged in Istanbul to date. Four teams, Bİ'ŞEYLER New Media Works, OUCHHH, Panpiper and Staras came together and set out to explore constellation Cygnus, the Swan, which is home to Cygnus X-1, a galactic X-ray source believed to be a stellar mass black hole. The light installation was performed in a 2400-m2 venue on December 18-19, 2014 in Istanbul. Using 46 Clay Paky Sharpies and 2 Atmosphere Hazers, the performance immersed 2000 viewers in the experience of the constellation which is believed to be about 5 million years old. Light sources were placed to surround the audience at different heights to allow light flow above their heads, creating a void at the center which prompted viewers to interpret the notion of a black hole. ...
In this animation, exoplanet HD 189733b is seen in closeup as it passes in front of its parent star. Hubble observed the planet do this in 2010 and 2011. This simulation depicts the 2011 observations, in which the planet’s atmosphere is evaporating away, possibly under the influence of a stellar flare. In this video, the surface of the star, which is around 80% the mass of the Sun, is animated based on observations of the Sun from the Solar Dynamics Observatory. Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory More information and download-options: http://www.spacetelescope.org/videos/heic1209c/
CROWDFUNDING NOW RUNNING: http://theriseofthesynths.com/crowdfunding The Rise of the Synths is a documentary about the Synthwave scene, nostalgia and the universe of creating sounds. 'The old soundtrack of a new generation' The film is a time travel towards the roots of a worldwide grass-root music scene known as Synthwave, an irresistible blending of modern electronic composition with 80s pop culture’s nostalgia, that over the last two years has transformed from a whisper on selected internet hubs, to a ever-growing scene expanding rapidly as we speak. Accounting millions of plays on social media, devoted fans are legion, but nobody in the mass media knows about them. A time travel into the universe of creating sounds. A love letter to human fascination and the collective memories of...
music by Lucas Thanos images by various artists Black and White Holes A black hole is a mathematically defined region of spacetime exhibiting such a strong gravitational pull that no particle or electromagnetic radiation can escape from it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which no escape is possible is called the event horizon. Although crossing the event horizon has enormous effect on the fate of the object crossing it, it appears to have no locally detectable features. In many ways a black hole acts like an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spec...
CROWDFUNDING NOW RUNNING: http://theriseofthesynths.com/crowdfunding Featuring: Electric Youth, College, Miami Nights 1984, Stellar Dreams, Dance with the dead, Power Glove, Nightcrawler Music, Vincenzo Salvia, Com Truise, The Midnight, Maethelvin, Jordan F, Betamaxx, Futurecop!, Dynatron, Lazerhawk, mitch murder, Darkest, OGRE, Kristine, Carpenter Brut, Timecop1983, Waveshaper, MPM Soundtracks. "A genius is a fool, until his idea succeeds..." You can make this dream come true. The Rise of the Synths is a documentary (and a time travel) about the SynthWave scene. 'The old sountrack of a new generation' The film is a time travel towards the roots of a worldwide grass-root music scene known as Synthwave, an irresistible blending of modern electronic composition with 80s pop culture’s n...
Because No Man's Sky isn't here yet.
A stellar black hole (or stellar-mass black hole) is a black hole formed by the gravitational collapse of a massive star. They have masses ranging from about 5 to several tens of solar masses. The process is observed as a hypernova explosion or as a gamma ray burst. These black holes are also referred to as collapsars.
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Heidelberg Joint Astronomical Colloquium