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Images of 'Onde De Choc' found, 65

Shock wave, 2008 (computer graphics)
 
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Shock wave, 2008 (computer graphics)

Ong, Diana (b.1940)

SSI2195671

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Shock wave, 2008 (computer graphics)

Ong, Diana (b.1940)

SSI2195671

Trees fall from the shock wave of a Soviet nuclear test at the Totskoye test site, USSR, 1954
 
Trees fall from the shock wave of a Soviet nuclear test at the Totskoye test site, USSR, 1954

TME3619021

Trees fall from the shock wave of a Soviet nuclear test at the Totskoye test site, USSR, 1954

TME3619021

Shock waves and destruction from Soviet nuclear bomb testing, 1950s
 
Shock waves and destruction from Soviet nuclear bomb testing, 1950s

TME3619023

Shock waves and destruction from Soviet nuclear bomb testing, 1950s

TME3619023

MAXI YACHT SHOCKWAVE LEADS WILD THING OUT OF SYDNEY HEADS AFTER START OF SYDNEY TO HOBART YACHT RACE, 2000-12-26 (photo)
 
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MAXI YACHT SHOCKWAVE LEADS WILD THING OUT OF SYDNEY HEADS AFTER START OF SYDNEY TO HOBART YACHT RACE, 2000-12-26 (photo)

Will Burgess

REU7818973

MAXI YACHT SHOCKWAVE LEADS WILD THING OUT OF SYDNEY HEADS AFTER START OF SYDNEY TO HOBART YACHT RACE, 2000-12-26 (photo)

Will Burgess

REU7818973

Aftermath of nuclear bomb test, USSR 1954
 
Aftermath of nuclear bomb test, USSR 1954

TME3619043

Aftermath of nuclear bomb test, USSR 1954

TME3619043

Cygnus Loop supernova blast wave, 1993
 
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Cygnus Loop supernova blast wave, 1993

UIS5093381

Cygnus Loop supernova blast wave, 1993

UIS5093381

Probably the first Soviet experiment of an atomic bomb, RDS-1, 29 August 1949
 
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Probably the first Soviet experiment of an atomic bomb, RDS-1, 29 August 1949

FLM3100382

Probably the first Soviet experiment of an atomic bomb, RDS-1, 29 August 1949

FLM3100382

Nuclear 'Operation Cue' tested structures' ability to survive atomic bombs. Bottom image shows a disintegrating shed beside liquefied petroleum tank as blast wave hits. April 4, 1955
 
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Nuclear 'Operation Cue' tested structures' ability to survive atomic bombs. Bottom image shows a disintegrating shed beside liquefied petroleum tank as blast wave hits. April 4, 1955

EVB2942430

Nuclear 'Operation Cue' tested structures' ability to survive atomic bombs. Bottom image shows a disintegrating shed beside liquefied petroleum tank as blast wave hits. April 4, 1955

EVB2942430

Franklin Delano Roosevelt; Harry S. Truman is sworn in as president of US, Albert Einstein, Julius Robert Oppenheimer, atomic experiment
 
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Franklin Delano Roosevelt; Harry S. Truman is sworn in as president of US, Albert Einstein, Julius Robert Oppenheimer, atomic experiment

IMW1121843

Franklin Delano Roosevelt; Harry S. Truman is sworn in as president of US, Albert Einstein, Julius Robert Oppenheimer, atomic experiment

IMW1121843

Operation Buster-Jangle nuclear bomb test, Nevada Test Site, USA 1951
 
Operation Buster-Jangle nuclear bomb test, Nevada Test Site, USA 1951

TME3619042

Operation Buster-Jangle nuclear bomb test, Nevada Test Site, USA 1951

TME3619042

The BAKER test of Operation Crossroads was exploded underwater on July 25, 1946. Image shows condensation cloud and air shock wave moving over the water and target ships. BAKER detonation illuminated the water from beneath the surface with an underwater fireball
 
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The BAKER test of Operation Crossroads was exploded underwater on July 25, 1946. Image shows condensation cloud and air shock wave moving over the water and target ships. BAKER detonation illuminated the water from beneath the surface with an underwater fireball

EVB2947971

The BAKER test of Operation Crossroads was exploded underwater on July 25, 1946. Image shows condensation cloud and air shock wave moving over the water and target ships. BAKER detonation illuminated the water from beneath the surface with an underwater fireball

EVB2947971

The BAKER test of Operation Crossroads, July 25, 1946. Photo shows the dome shaped condensation cloud around the gas bubble of the fireball
 
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The BAKER test of Operation Crossroads, July 25, 1946. Photo shows the dome shaped condensation cloud around the gas bubble of the fireball

EVB2948050

The BAKER test of Operation Crossroads, July 25, 1946. Photo shows the dome shaped condensation cloud around the gas bubble of the fireball

EVB2948050

The BAKER test of Operation Crossroads, July 25, 1946. The fireball and water column emerge from the dome of condensation cloud less than two seconds after the detonation
 
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The BAKER test of Operation Crossroads, July 25, 1946. The fireball and water column emerge from the dome of condensation cloud less than two seconds after the detonation

EVB2948061

The BAKER test of Operation Crossroads, July 25, 1946. The fireball and water column emerge from the dome of condensation cloud less than two seconds after the detonation

EVB2948061

Hiroshima bomb explosion, devastation, casualties, Emperor Hiroito as Japan surrenders, test of the first hydrogen bomb
 
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Hiroshima bomb explosion, devastation, casualties, Emperor Hiroito as Japan surrenders, test of the first hydrogen bomb

IMW1121783

Hiroshima bomb explosion, devastation, casualties, Emperor Hiroito as Japan surrenders, test of the first hydrogen bomb

IMW1121783

The STOKES shot was a 19 kiloton explosion detonated while suspended from barrage balloons. The wrecked Navy Goodyear Blimp had been in free flight over 5 miles form ground zero when destroyed collapsed by the blast's shock wave. Nevada test Site, August 7, 1957
 
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The STOKES shot was a 19 kiloton explosion detonated while suspended from barrage balloons. The wrecked Navy Goodyear Blimp had been in free flight over 5 miles form ground zero when destroyed collapsed by the blast's shock wave. Nevada test Site, August 7, 1957

EVB2942426

The STOKES shot was a 19 kiloton explosion detonated while suspended from barrage balloons. The wrecked Navy Goodyear Blimp had been in free flight over 5 miles form ground zero when destroyed collapsed by the blast's shock wave. Nevada test Site, August 7, 1957

EVB2942426

Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure
 
Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

PIX4583800

Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

PIX4583800

Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure
 
Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

PIX4583806

Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure

PIX4583806

A TRADER SPEAKS ON THE PHONE IN MICEX, 1998-08-28 (photo)
 
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A TRADER SPEAKS ON THE PHONE IN MICEX, 1998-08-28 (photo)

Viktor Korotayev

REU8033669

A TRADER SPEAKS ON THE PHONE IN MICEX, 1998-08-28 (photo)

Viktor Korotayev

REU8033669

STUDENTS PAY RESPECT TO MOTHER TERESA IN DHAKA, 1997-09-08 (photo)
 
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STUDENTS PAY RESPECT TO MOTHER TERESA IN DHAKA, 1997-09-08 (photo)

Rafiquar Rahman

REU8044947

STUDENTS PAY RESPECT TO MOTHER TERESA IN DHAKA, 1997-09-08 (photo)

Rafiquar Rahman

REU8044947

EMPLOYEES OF THE CREDIT SUISSE BANK, 1997-10-27 (photo)
 
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EMPLOYEES OF THE CREDIT SUISSE BANK, 1997-10-27 (photo)

Andy Mueller

REU7907913

EMPLOYEES OF THE CREDIT SUISSE BANK, 1997-10-27 (photo)

Andy Mueller

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AN EMPLOYEE OF CREDIT SUISSE BANK WATCHES COMPUTER MONITOR, 1997-10-27 (photo)
 
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AN EMPLOYEE OF CREDIT SUISSE BANK WATCHES COMPUTER MONITOR, 1997-10-27 (photo)

Andy Mueller

REU7907645

AN EMPLOYEE OF CREDIT SUISSE BANK WATCHES COMPUTER MONITOR, 1997-10-27 (photo)

Andy Mueller

REU7907645

Speeches in the Kremlin on the occasion of the 60th anniversary of the USSR, 1982
 
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Speeches in the Kremlin on the occasion of the 60th anniversary of the USSR, 1982

FLM3084864

Speeches in the Kremlin on the occasion of the 60th anniversary of the USSR, 1982

FLM3084864

Employees of Switzerland's Credit Suisse bank make telephone calls as they sit in front of computer.., 1997-10-27 (photo)
 
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Employees of Switzerland's Credit Suisse bank make telephone calls as they sit in front of computer.., 1997-10-27 (photo)

Andy Mueller

REU7646818

Employees of Switzerland's Credit Suisse bank make telephone calls as they sit in front of computer.., 1997-10-27 (photo)

Andy Mueller

REU7646818

EMPLOYEES OF CREDIT SUISSE BANK ON PHONES, 1997-10-27 (photo)
 
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EMPLOYEES OF CREDIT SUISSE BANK ON PHONES, 1997-10-27 (photo)

Andy Mueller

REU7970317

EMPLOYEES OF CREDIT SUISSE BANK ON PHONES, 1997-10-27 (photo)

Andy Mueller

REU7970317

A SOUTH KOREAN STOCK INVESTOR READS A NEWSPAPER IN SEOUL, 2000-04-18 (photo)
 
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A SOUTH KOREAN STOCK INVESTOR READS A NEWSPAPER IN SEOUL, 2000-04-18 (photo)

Reuters Photographer

REU7764050

A SOUTH KOREAN STOCK INVESTOR READS A NEWSPAPER IN SEOUL, 2000-04-18 (photo)

Reuters Photographer

REU7764050

PICTURE TAKEN OF TWO OF PALESTINIAN BUILDINGS DESTROYED IN GAZA STRIP BY ISRAELI ARMY, 2003-10-24 (photo)
 
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PICTURE TAKEN OF TWO OF PALESTINIAN BUILDINGS DESTROYED IN GAZA STRIP BY ISRAELI ARMY, 2003-10-24 (photo)

Tsafrir Abayov

REU8029053

PICTURE TAKEN OF TWO OF PALESTINIAN BUILDINGS DESTROYED IN GAZA STRIP BY ISRAELI ARMY, 2003-10-24 (photo)

Tsafrir Abayov

REU8029053

ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION PRESIDENT PRODI IN ROME., 2003-07-04 (photo)
 
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ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION PRESIDENT PRODI IN ROME., 2003-07-04 (photo)

Giampiero Sposito

REU7574499

ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION PRESIDENT PRODI IN ROME., 2003-07-04 (photo)

Giampiero Sposito

REU7574499

EMPLOYEES OF A BROKERAGE OFFICE LEAVE BUILDING FOLLOWING BLAST IN CYPRUS, 2000-08-08 (photo)
 
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EMPLOYEES OF A BROKERAGE OFFICE LEAVE BUILDING FOLLOWING BLAST IN CYPRUS, 2000-08-08 (photo)

Reuters Photographer

REU7723954

EMPLOYEES OF A BROKERAGE OFFICE LEAVE BUILDING FOLLOWING BLAST IN CYPRUS, 2000-08-08 (photo)

Reuters Photographer

REU7723954

A SOUTH KOREAN INVESTOR MONITORS STOCK PRICES IN SEOUL, 2000-04-17 (photo)
 
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A SOUTH KOREAN INVESTOR MONITORS STOCK PRICES IN SEOUL, 2000-04-17 (photo)

Reuters Photographer

REU7978964

A SOUTH KOREAN INVESTOR MONITORS STOCK PRICES IN SEOUL, 2000-04-17 (photo)

Reuters Photographer

REU7978964

Sony Style.com Japan Inc President Kazumasa Sato speaks during a news conference held at Sony headqu.., 2000 (photo)
 
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Sony Style.com Japan Inc President Kazumasa Sato speaks during a news conference held at Sony headqu.., 2000 (photo)

Kimimasa Mayama

REU7475030

Sony Style.com Japan Inc President Kazumasa Sato speaks during a news conference held at Sony headqu.., 2000 (photo)

Kimimasa Mayama

REU7475030

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)
 
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SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7643666

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7643666

The BAKER test of Operation Crossroads, July 25, 1946
 
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The BAKER test of Operation Crossroads, July 25, 1946

EVB2948072

The BAKER test of Operation Crossroads, July 25, 1946

EVB2948072

ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION IN ROME, 2003-07-04 (photo)
 
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ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION IN ROME, 2003-07-04 (photo)

Giampiero Sposito

REU7872412

ITALIAN PREMIER BERLUSCONI MEETS EUROPEAN COMMISSION IN ROME, 2003-07-04 (photo)

Giampiero Sposito

REU7872412

PALESTINIAN BOY SITS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)
 
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PALESTINIAN BOY SITS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU8034438

PALESTINIAN BOY SITS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU8034438

YOKOHAMA MAYOR NAKADA SPEAKS TO REPORTERS IN TOKYO, 2002-07-04 (photo)
 
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YOKOHAMA MAYOR NAKADA SPEAKS TO REPORTERS IN TOKYO, 2002-07-04 (photo)

Eriko Sugita

REU7919861

YOKOHAMA MAYOR NAKADA SPEAKS TO REPORTERS IN TOKYO, 2002-07-04 (photo)

Eriko Sugita

REU7919861

Tunguska valley - Artist view (2/3)
 
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Tunguska valley - Artist view (2/3)

PIX4583789

Tunguska valley - Artist view (2/3)

PIX4583789

SONY STYLE.COM PRESIDENT KAZUMASA SATO SPEAKS IN TOKYO, 2000-02-01 (photo)
 
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SONY STYLE.COM PRESIDENT KAZUMASA SATO SPEAKS IN TOKYO, 2000-02-01 (photo)

Kimimasa Mayama

REU7711378

SONY STYLE.COM PRESIDENT KAZUMASA SATO SPEAKS IN TOKYO, 2000-02-01 (photo)

Kimimasa Mayama

REU7711378

Sony Corp Vice President Junichi Kodera listens to a question form a reporter during a news conferen.., 2000 (photo)
 
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Sony Corp Vice President Junichi Kodera listens to a question form a reporter during a news conferen.., 2000 (photo)

Kimimasa Mayama

REU7475029

Sony Corp Vice President Junichi Kodera listens to a question form a reporter during a news conferen.., 2000 (photo)

Kimimasa Mayama

REU7475029

Fusee Ariane 5 ECA - 07/2009 - Ariane 5 ECA V189 lift off - 07/2009 - Decolving the Ariane 5 ECA rocket with the TerreStar telecommunication satellite on board on 1 July 2009. A shock wave appears as the sound wall passes. Lift - off of flight V189 took place 1 July 2009 at 19:52 CEST/Paris (17:52 UTC/GMT; 14:52 UTC - 3/English Guiana) The target orbit had a perigee altitude of 250 km, an apogee altitude at injection of 35 786 km and an inclination of six degrees. TerreStar 1 was accurately injected into its transfer orbit about 26 minutes after lift - off. Here, a shockwave forms as Ariane 5 roars through the sound barrier. TerreStar 1 will be the largest and most powerful commercial telecommunications satellite ever launched and will provide voice, data and video communications to satellite
 
Fusee Ariane 5 ECA - 07/2009 - Ariane 5 ECA V189 lift off - 07/2009 - Decolving the Ariane 5 ECA rocket with the TerreStar telecommunication satellite on board on 1 July 2009. A shock wave appears as the sound wall passes. Lift - off of flight V189 took place 1 July 2009 at 19:52 CEST/Paris (17:52 UTC/GMT; 14:52 UTC - 3/English Guiana) The target orbit had a perigee altitude of 250 km, an apogee altitude at injection of 35 786 km and an inclination of six degrees. TerreStar 1 was accurately injected into its transfer orbit about 26 minutes after lift - off. Here, a shockwave forms as Ariane 5 roars through the sound barrier. TerreStar 1 will be the largest and most powerful commercial telecommunications satellite ever launched and will provide voice, data and video communications to satellite

S. Corvaja

PIX4604359

Fusee Ariane 5 ECA - 07/2009 - Ariane 5 ECA V189 lift off - 07/2009 - Decolving the Ariane 5 ECA rocket with the TerreStar telecommunication satellite on board on 1 July 2009. A shock wave appears as the sound wall passes. Lift - off of flight V189 took place 1 July 2009 at 19:52 CEST/Paris (17:52 UTC/GMT; 14:52 UTC - 3/English Guiana) The target orbit had a perigee altitude of 250 km, an apogee altitude at injection of 35 786 km and an inclination of six degrees. TerreStar 1 was accurately injected into its transfer orbit about 26 minutes after lift - off. Here, a shockwave forms as Ariane 5 roars through the sound barrier. TerreStar 1 will be the largest and most powerful commercial telecommunications satellite ever launched and will provide voice, data and video communications to satellite

S. Corvaja

PIX4604359

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)
 
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SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7711121

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7711121

Tungouska event -Artist view (1/3)
 
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Tungouska event -Artist view (1/3)

PIX4583779

Tungouska event -Artist view (1/3)

PIX4583779

JAPANESE MAN USES CELL PHONE IN FRONT OF STOCK QUOTATION BOARD IN TOKYO, 2001-09-12 (photo)
 
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JAPANESE MAN USES CELL PHONE IN FRONT OF STOCK QUOTATION BOARD IN TOKYO, 2001-09-12 (photo)

Eriko Sugita

REU7973340

JAPANESE MAN USES CELL PHONE IN FRONT OF STOCK QUOTATION BOARD IN TOKYO, 2001-09-12 (photo)

Eriko Sugita

REU7973340

VIPs view the DOG shot, an 81 kiloton atomic detonation wearing safety goggles
 
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VIPs view the DOG shot, an 81 kiloton atomic detonation wearing safety goggles

EVB2947927

VIPs view the DOG shot, an 81 kiloton atomic detonation wearing safety goggles

EVB2947927

Tunguska valley - Artist view (3/3)
 
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Tunguska valley - Artist view (3/3)

PIX4583798

Tunguska valley - Artist view (3/3)

PIX4583798

ATOMIC BOMB HIROSHIMA Shortly after 8:15 am. 6th August 1945. Looking …, 1945 (photo)
 
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ATOMIC BOMB HIROSHIMA Shortly after 8:15 am. 6th August 1945. Looking …, 1945 (photo)

IMO8740498

ATOMIC BOMB HIROSHIMA Shortly after 8:15 am. 6th August 1945. Looking …, 1945 (photo)

IMO8740498

A STOCK MARKET INVESTOR IN TAIWAN, 1997-10-24 (photo)
 
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A STOCK MARKET INVESTOR IN TAIWAN, 1997-10-24 (photo)

Simon Kwong

REU8011787

A STOCK MARKET INVESTOR IN TAIWAN, 1997-10-24 (photo)

Simon Kwong

REU8011787

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova Kepler in Ophiuchus - Kepler's supernova remnant
 
Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

PIX4626476

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

PIX4626476

Financial Services Minister Hakuo Yanagisawa speaks to reporters at his ministry in Tokyo September ..., 2002 (photo)
 
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Financial Services Minister Hakuo Yanagisawa speaks to reporters at his ministry in Tokyo September ..., 2002 (photo)

Eriko Sugita

REU7454017

Financial Services Minister Hakuo Yanagisawa speaks to reporters at his ministry in Tokyo September ..., 2002 (photo)

Eriko Sugita

REU7454017

A BUTCHER CUTS A PIECE OF ITALIAN BEEF MEAT IN ROME, 2000-11-15 (photo)
 
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A BUTCHER CUTS A PIECE OF ITALIAN BEEF MEAT IN ROME, 2000-11-15 (photo)

Alessia Pierdomenico

REU7879666

A BUTCHER CUTS A PIECE OF ITALIAN BEEF MEAT IN ROME, 2000-11-15 (photo)

Alessia Pierdomenico

REU7879666

PALESTINIANS INSPECT THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)
 
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PALESTINIANS INSPECT THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU7857827

PALESTINIANS INSPECT THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU7857827

FILE PHOTO OF WISCONSIN BISHOP RICHARD J SKLBA, 2002-05-18 (photo)
 
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FILE PHOTO OF WISCONSIN BISHOP RICHARD J SKLBA, 2002-05-18 (photo)

Allen Fredrickson

REU7918512

FILE PHOTO OF WISCONSIN BISHOP RICHARD J SKLBA, 2002-05-18 (photo)

Allen Fredrickson

REU7918512

Photograph shows WorldCom sign at the company's facility in Ashburn, VA, June 26, 2002 (photo)
 
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Photograph shows WorldCom sign at the company's facility in Ashburn, VA, June 26, 2002 (photo)

Win McNamee

REU7454027

Photograph shows WorldCom sign at the company's facility in Ashburn, VA, June 26, 2002 (photo)

Win McNamee

REU7454027

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)
 
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SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7642510

SONY STARTS SELLING CONSUMER ELECTRONICS ONLINE, 2000-02-01 (photo)

Kimimasa Mayama

REU7642510

WORLDCOM HEADQUARTERS BUILDING IN MISSISSIPPI, 2002-06-25 (photo)
 
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WORLDCOM HEADQUARTERS BUILDING IN MISSISSIPPI, 2002-06-25 (photo)

Suzi Altman

REU7954263

WORLDCOM HEADQUARTERS BUILDING IN MISSISSIPPI, 2002-06-25 (photo)

Suzi Altman

REU7954263

PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)
 
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PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU8034426

PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU8034426

JAPAN'S FINANCIAL SERVICES MINISTER YANAGISAWA SPEAKS TO REPORTERS IN TOKYO, 2002-09-18 (photo)
 
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JAPAN'S FINANCIAL SERVICES MINISTER YANAGISAWA SPEAKS TO REPORTERS IN TOKYO, 2002-09-18 (photo)

Eriko Sugita

REU8064205

JAPAN'S FINANCIAL SERVICES MINISTER YANAGISAWA SPEAKS TO REPORTERS IN TOKYO, 2002-09-18 (photo)

Eriko Sugita

REU8064205

WORLDCOM FACILITY IN ASHBURN VIRGINIA, 2002-06-26 (photo)
 
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WORLDCOM FACILITY IN ASHBURN VIRGINIA, 2002-06-26 (photo)

Win McNamee

REU7801603

WORLDCOM FACILITY IN ASHBURN VIRGINIA, 2002-06-26 (photo)

Win McNamee

REU7801603

PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)
 
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PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU7917503

PALESTINIAN BOY WALKS ON RUBBLE OF THREE BUILDINGS DESTROYED BY ISRAELI ARMY IN GAZA STRIP, 2003-10-26 (photo)

Suhaib Salem

REU7917503

Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding material to collapse into dense clumps that are the birthplaces of new stars. The region, called RCW120, is about 4200 light years from Earth, towards the constellation of Scorpius. A hot, massive star in its centre is emitting huge amounts of ultraviolet radiation, which ionises the surrounding gas, stripping the electrons from hydrogen atoms and producing the characteristic red glow of so - called H - alpha emission. Here, the submillimetre emission is shown as the blue clouds surrounding the reddish glow of the ionised gas (shown with data from the SuperCosmoS H - alpha survey). The image also contains data from the Second Generation Digitized Sky Survey (I - band shown in blue, R - band shown in red). As this ionised region expands into space, the associated shock wave sweeps up a layer of the surrounding cold interstellar gas and cosmic dust. This layer b
 
Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding mat

PIX4621694

Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding mat

PIX4621694

CHILDREN PASS CLOSED WORLDCOM STORE, 2002-06-26 (photo)
 
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CHILDREN PASS CLOSED WORLDCOM STORE, 2002-06-26 (photo)

Brian Snyder

REU7911425

CHILDREN PASS CLOSED WORLDCOM STORE, 2002-06-26 (photo)

Brian Snyder

REU7911425

Ernst Mach, Austrian physicist and philosopher, c 1910
 
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Ernst Mach, Austrian physicist and philosopher, c 1910

UIS5071955

Ernst Mach, Austrian physicist and philosopher, c 1910

UIS5071955

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dimensional structure. The filamentary emission has a very distinct boundary on the side facing away from LL Ori, but is diffuse on the side closest to the star, a characteristic common to many bow shocks. A second, fainter bow shock can be seen around a star near the upper right - hand corner of the image. Astronomers have identified numerous shock fronts in this complex star - forming region and are using this data to understand the many complex phenomena associated with the birth of stars. This image was taken in February 1995 as part of the Hubble Orion Nebula mosaic. A close visitor in our Milky Way galaxy, the nebula is only 1,500 light - years from Earth. The filters used in this color composite represent oxygen, nitrogen, and hydrogen emissions
 
Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part of a binary star system with an even more massive partner. It's believed that when the partner exploded as a supernova, blasting away most of its mass, Zeta Ophiuchi was suddenly freed from its partner's pull and shot away like a bullet moving 24 kilometers per second (54,000 miles per hour). Zeta Ophiuchi is about 20 times more massive and 65,000 times more luminous than the sun. If it werenn't surrounded by so much dust, it would be one of the brightest stars in the sky and appear blue to the eye. Like all stars with this kind of extreme mass and power, it subscribes to the 'live fast, die young' motto. It's already about halfway through its very short 8 - million - year lifespan. In comparison, the sun is roughly halfway through its 10 - billion - year lifespan. While the sun will eventually become a quiet white dwarf, Zeta Ophiuchi, like its ex - partner, will ultimately die in a massive explosion called a supernova. Perhaps t
 
Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

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