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'Gravitational Wave' Bilder und Clips Suchergebnisse page 1 of 1

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Bilder zu 'Gravitational Wave' gefunden, 20

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe
 
Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

PIX4607586

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of two colliding neutron stars about to merge and explode in kilonova. This type of event produces gravitational waves and a gamma ray burst. This artist's impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. Such a very rare event is expected to produce both gravitational waves and a short gamma-ray burst, both of which were observed on 17 August 2017 by LIGO-Virgo and Fermi/INTEGRAL respectively. Subsequent detailed observations with many ESO telescopes confirmed that this object, seen in the galaxy NGC 4993 about 130 million light-years from the Earth, is indeed a kilonova. Such objects are the main source of very heavy chemical elements, such as gold and platinum, in the Universe

PIX4607586

Gravitational Waves - Gravitational Waves: Two colliding neutron stars create a gravitational wave that spreads over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017.
 
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Gravitational Waves - Gravitational Waves: Two colliding neutron stars create a gravitational wave that spreads over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017.

Dixon, Don (b.1951)

PIX4607592

Gravitational Waves - Gravitational Waves: Two colliding neutron stars create a gravitational wave that spreads over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017.

Dixon, Don (b.1951)

PIX4607592

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale
 
Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

PIX4572892

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

PIX4572892

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of a gravitational wave generated by a system of two neutron stars in collision, spreading over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017. A couple of seconds after that, ESA's Integral and Nasa's Fermi satellites detected a burst of gamma rays, the luminous counterpart to the gravitational waves emitted by the cosmic clash. This is the first discovery of gravitational waves and light coming from the same source
 
Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of a gravitational wave generated by a system of two neutron stars in collision, spreading over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017. A couple of seconds after that, ESA's Integral and Nasa's Fermi satellites detected a burst of gamma rays, the luminous counterpart to the gravitational waves emitted by the cosmic clash. This is the first discovery of gravitational waves and light coming from the same source

PIX4607575

Colliding neutron stars and gravitational waves - Colliding neutron stars and gravitational waves: Artist's view of a gravitational wave generated by a system of two neutron stars in collision, spreading over the space-time fabric. Artist's impression of two neutron stars - the compact remnants of what were once massive stars - spiralling towards each other just before merging. The collision of these dense, compact objects produced gravitational waves - fluctuations in the fabric of spacetime - that were detected by the LIGO/Virgo collaboration on 17 August 2017. A couple of seconds after that, ESA's Integral and Nasa's Fermi satellites detected a burst of gamma rays, the luminous counterpart to the gravitational waves emitted by the cosmic clash. This is the first discovery of gravitational waves and light coming from the same source

PIX4607575

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale
 
Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

PIX4572795

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right, it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves (shown as the grid in this picture) cannot be yet detected directly by astronomers on Earth they can be sensed indirectly by measuring the change in the orbit of

PIX4572795

Gravitational waves
 
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Gravitational waves

Miller, Ron (b.1947)

PIX7223397

Gravitational waves

Miller, Ron (b.1947)

PIX7223397

PHOTO TAKEN 09JAN02-Scientific technician Bartie Rivera does an operational check on an educational.., 2002 (photo)
 
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PHOTO TAKEN 09JAN02-Scientific technician Bartie Rivera does an operational check on an educational.., 2002 (photo)

Anthony P. Bolante

REU7464510

PHOTO TAKEN 09JAN02-Scientific technician Bartie Rivera does an operational check on an educational.., 2002 (photo)

Anthony P. Bolante

REU7464510

Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIGO Hanford Observatory.., 2002-01-18 (photo)
 
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Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIGO Hanford Observatory.., 2002-01-18 (photo)

Anthony P. Bolante

REU7510781

Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIGO Hanford Observatory.., 2002-01-18 (photo)

Anthony P. Bolante

REU7510781

Bob Coldwell of the University of Florida conducts research while sitting near monitors showing the .., 2002 (photo)
 
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Bob Coldwell of the University of Florida conducts research while sitting near monitors showing the .., 2002 (photo)

Anthony P. Bolante

REU7455880

Bob Coldwell of the University of Florida conducts research while sitting near monitors showing the .., 2002 (photo)

Anthony P. Bolante

REU7455880

PHOTO TAKEN 09JAN02-Concrete and stainless steel tubes house and protect the four-kilometer long la.., 2002 (photo)
 
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PHOTO TAKEN 09JAN02-Concrete and stainless steel tubes house and protect the four-kilometer long la.., 2002 (photo)

Anthony P. Bolante

REU7464520

PHOTO TAKEN 09JAN02-Concrete and stainless steel tubes house and protect the four-kilometer long la.., 2002 (photo)

Anthony P. Bolante

REU7464520

PHOTO TAKEN 09JAN02-Dr. Fred Raab, observatory head at the LIGO Hanford Observatory in Hanford, Was.., 2002 (photo)
 
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PHOTO TAKEN 09JAN02-Dr. Fred Raab, observatory head at the LIGO Hanford Observatory in Hanford, Was.., 2002 (photo)

Anthony P. Bolante

REU7460730

PHOTO TAKEN 09JAN02-Dr. Fred Raab, observatory head at the LIGO Hanford Observatory in Hanford, Was.., 2002 (photo)

Anthony P. Bolante

REU7460730

LIGO HANFORD FACILITY RESEARCHER WITH EDUCATIONAL LASER DISPLAY, 2002-01-09 (photo)
 
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LIGO HANFORD FACILITY RESEARCHER WITH EDUCATIONAL LASER DISPLAY, 2002-01-09 (photo)

Anthony P. Bolante

REU7806382

LIGO HANFORD FACILITY RESEARCHER WITH EDUCATIONAL LASER DISPLAY, 2002-01-09 (photo)

Anthony P. Bolante

REU7806382

PHOTO TAKEN 09JAN02-Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIG.., 2002-01-18 (photo)
 
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PHOTO TAKEN 09JAN02-Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIG.., 2002-01-18 (photo)

Anthony P. Bolante

REU7504641

PHOTO TAKEN 09JAN02-Wearing laser protective eyeglasses, Dr. Fred Raab, observatory head at the LIG.., 2002-01-18 (photo)

Anthony P. Bolante

REU7504641

CONCRETE TUBES PROTECT RESEARCH LASERS AT LIGO HANFORD RESEARCH FACILITY, 2002-01-09 (photo)
 
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CONCRETE TUBES PROTECT RESEARCH LASERS AT LIGO HANFORD RESEARCH FACILITY, 2002-01-09 (photo)

Anthony P. Bolante

REU7825521

CONCRETE TUBES PROTECT RESEARCH LASERS AT LIGO HANFORD RESEARCH FACILITY, 2002-01-09 (photo)

Anthony P. Bolante

REU7825521

SCIENTISTS AT LIGO FACILITY IN HANFORD WASHINGTON MONITOR LASERS, 2002-01-09 (photo)
 
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Nutzungsbeschränkungen von unseren Content-Partnern
  • Minimum fee applies to this image;Only available to clients invoiced in Australia, Belgium, Brazil, Bulgaria, Canada, China, Cyprus, Czech Republic, Estonia, Finland, France, French Southern Territories, Greece, Hong Kong, Hungary, India, Ireland, Israel, Italy, Lebanon, Luxembourg, Mexico, the Netherlands, New Zealand, Portugal, Qatar, Republic of Korea, Romania, Russian Federation, Singapore, South Africa, Spain, Sweden, Switzerland, Taiwan, Turkey, United Arab Emirates, United Kingdom and United States
SCIENTISTS AT LIGO FACILITY IN HANFORD WASHINGTON MONITOR LASERS, 2002-01-09 (photo)

Anthony P. Bolante

REU7880150

SCIENTISTS AT LIGO FACILITY IN HANFORD WASHINGTON MONITOR LASERS, 2002-01-09 (photo)

Anthony P. Bolante

REU7880150

DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS LASER APPARATUSES, 2002-01-09 (photo)
 
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Nutzungsbeschränkungen von unseren Content-Partnern
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DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS LASER APPARATUSES, 2002-01-09 (photo)

Anthony P. Bolante

REU7825534

DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS LASER APPARATUSES, 2002-01-09 (photo)

Anthony P. Bolante

REU7825534

DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS TUBES PROTECTING LASERS, 2002-01-09 (photo)
 
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  • Permission required for non-editorial use (inc book covers). Please contact us
Bildbeschränkungen
  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Nutzungsbeschränkungen von unseren Content-Partnern
  • Minimum fee applies to this image;Only available to clients invoiced in Australia, Belgium, Brazil, Bulgaria, Canada, China, Cyprus, Czech Republic, Estonia, Finland, France, French Southern Territories, Greece, Hong Kong, Hungary, India, Ireland, Israel, Italy, Lebanon, Luxembourg, Mexico, the Netherlands, New Zealand, Portugal, Qatar, Republic of Korea, Romania, Russian Federation, Singapore, South Africa, Spain, Sweden, Switzerland, Taiwan, Turkey, United Arab Emirates, United Kingdom and United States
DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS TUBES PROTECTING LASERS, 2002-01-09 (photo)

Anthony P. Bolante

REU7875519

DR FRED RAAB OF LIGO HANFORD FACILITY INSPECTS TUBES PROTECTING LASERS, 2002-01-09 (photo)

Anthony P. Bolante

REU7875519

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