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LEPIDUS EJECTED

LEPIDUS EJECTED

EPL6914606

Village squire ejected from cottage

Village squire ejected from cottage

EPL6919905

EJECTED FROM PUB, 1891

EJECTED FROM PUB, 1891

May, Philip William (1864-1903)

EPL6853827

ADAM & EVE EJECTED

ADAM & EVE EJECTED

Dore, Gustave (1832-83)

EPL6776949

Fish Ejected from Volcanoes (engraving)

Fish Ejected from Volcanoes (engraving)

English School, (19th century)

LLM3627880

Overtaxed subjects ejected from their homes, 1920's (litho)

Overtaxed subjects ejected from their homes, 1920's (litho)

Woodville, Richard Caton II (1856-1927)

IL833040

John Welch ejected from Irongray (engraving)

John Welch ejected from Irongray (engraving)

English School, (19th century)

LLM725585

Pilot being ejected from the Ryan XV-5 Jump Jet

Pilot being ejected from the Ryan XV-5 Jump Jet

Hardy, Wilf (Wilfred) (20th century)

LAL337361

Life in Parliament, Strangers in the House (engraving)

Life in Parliament, Strangers in the House (engraving)

Furniss, Harry (1854-1925) (after)

LIP1055464

There is a time to drink and a time to be chucked out (colour litho)

There is a time to drink and a time to be chucked out (colour litho)

English School, (20th century)

LLE813345

Large boulder ejected from Kepler crater.

Large boulder ejected from Kepler crater.

UIG866314

The Wonderful Adventures of Phra the Phoenician (engraving)

The Wonderful Adventures of Phra the Phoenician (engraving)

Paget, Henry Marriott (1856-1936) (after)

LIP1596655

SOCCER PLAYERS CHILAVERT AND BERMUDEZ EJECTED ARGENTINE LEAGUE MATCH, 2000-04-03 (photo)

SOCCER PLAYERS CHILAVERT AND BERMUDEZ EJECTED ARGENTINE LEAGUE MATCH, 2000-04-03 (photo)

Reuters Photographer

REU7764580

A PROTESTOR IS EJECTED FROM A FORD MEETING, 1997-05-08 (photo)

A PROTESTOR IS EJECTED FROM A FORD MEETING, 1997-05-08 (photo)

Reuters Photographer

REU7953135

A woman is ejected from the pews of the Foundling Hospital Chapel (coloured engraving)

A woman is ejected from the pews of the Foundling Hospital Chapel (coloured engraving)

English School, (19th century)

LLJ608838

Over-taxed subjects ejected from their houses, illustration from 'Hutchinson's Story of the British Nation', c.1923 (litho)

Over-taxed subjects ejected from their houses, illustration from 'Hutchinson's Story of the British Nation', c.1923 (litho)

Woodville, Richard Caton II (1856-1927) (after)

STC293137

John III Sobieski (1629-96) from 'Gallery of Portraits', published in 1833 (engraving)

John III Sobieski (1629-96) from 'Gallery of Portraits', published in 1833 (engraving)

English School, (19th century)

Ken Welsh

KWE189056

The Expulsion (oil on canvas)

The Expulsion (oil on canvas)

Hughes, Edward Robert (1851-1914)

BRA3664448

Window depicting Hagar and Ishmael, cast out by Abraham and Sarah, late 19th century (stained glass)

Window depicting Hagar and Ishmael, cast out by Abraham and Sarah, late 19th century (stained glass)

Preedy, Frederick (1820-98)

Neil Holmes

HGP3082432

VIKINGS RECEIVER MOSS EJECTED DURING LOSS TO BUCS, 2000-10-29 (photo)

VIKINGS RECEIVER MOSS EJECTED DURING LOSS TO BUCS, 2000-10-29 (photo)

Pierre Ducharme

REU7937314

BLUE JAYS FRASCATORE EJECTED WHILE ARGUING WITH UMPIRE, 2000-07-30 (photo)

BLUE JAYS FRASCATORE EJECTED WHILE ARGUING WITH UMPIRE, 2000-07-30 (photo)

Anthony P. Bolante

REU7929290

Path of projectile ejected at various velocities until sufficient to put it into orbit. From a English translation of Newton's ''Principia''.

Path of projectile ejected at various velocities until sufficient to put it into orbit. From a English translation of Newton's ''Principia''.

UIG865392

WHITE SOX PETTIS EJECTED BY UMPIRE CEDERSTROM, 2002-07-31 (photo)

WHITE SOX PETTIS EJECTED BY UMPIRE CEDERSTROM, 2002-07-31 (photo)

Eric Miller

REU8004663

Model depicting Mohandas Karamchand Gandhi ejected from a first class railway train, South Africa

Model depicting Mohandas Karamchand Gandhi ejected from a first class railway train, South Africa

Unknown photographer, (20th century)

UIG3586890

PHILLIES MANAGER BOWA EJECTED BY UMPIRE BARKSDALE, 2003-09-17 (photo)

PHILLIES MANAGER BOWA EJECTED BY UMPIRE BARKSDALE, 2003-09-17 (photo)

Tim Shaffer

REU7724027

The Strike of Colliers in Durham (engraving)

The Strike of Colliers in Durham (engraving)

English School, (19th century)

LIP1102893

Window Ew-L depicting a scene from the Prodigal Son story: he is thrown out by the coutesans (stained glass)

Window Ew-L depicting a scene from the Prodigal Son story: he is thrown out by the coutesans (stained glass)

French School, (13th century)

PC719905

Cross-section of Elihu Whitney's (1765-1825) saw-gin for cleaning cotton, 1865 (engraving)

Cross-section of Elihu Whitney's (1765-1825) saw-gin for cleaning cotton, 1865 (engraving)

UIG531565

DEVIL RAYS YAN EJECTED AFTER FIGHT WITH MARINERS MCLEMORE, 2000-05-20 (photo)

DEVIL RAYS YAN EJECTED AFTER FIGHT WITH MARINERS MCLEMORE, 2000-05-20 (photo)

Anthony Bolante

REU7929629

CARDINALS COACH OQUENDO EJECTED IN FOURTH INNING AGAINST CUBS, 2002-05-08 (photo)

CARDINALS COACH OQUENDO EJECTED IN FOURTH INNING AGAINST CUBS, 2002-05-08 (photo)

Sue Ogrocki

REU7948652

ORIOLES MANAGER MIKE HARGROVE EJECTED BY UMPIRE ANDY FLETCHER, 2003-07-06 (photo)

ORIOLES MANAGER MIKE HARGROVE EJECTED BY UMPIRE ANDY FLETCHER, 2003-07-06 (photo)

Joe Giza

REU7785487

INDIAN CAPTAIN GANGULY IS BOWLED OUT LBW FOR A DUCK BY ENGLAND'S
HOGGART DURING FOURTH DAY OF TEST, 2002-07-28 (photo) — INDIAN CAPTAIN GANGULY IS BOWLED OUT LBW FOR A DUCK BY ENGLAND'S HOGGART DURING FOURTH DAY OF TEST, 2002-07-28 (photo)

INDIAN CAPTAIN GANGULY IS BOWLED OUT LBW FOR A DUCK BY ENGLAND'S HOGGART DURING FOURTH DAY OF TEST, 2002-07-28 (photo)

Stephen Hird

REU7888698

ASTROS MANAGER JIMY WILLIAMS AND JEFF KENT EJECTED FOR ARGUING STRIKE
CALL, 2003-07-26 (photo) — ASTROS MANAGER JIMY WILLIAMS AND JEFF KENT EJECTED FOR ARGUING STRIKE CALL, 2003-07-26 (photo)

ASTROS MANAGER JIMY WILLIAMS AND JEFF KENT EJECTED FOR ARGUING STRIKE CALL, 2003-07-26 (photo)

Richard Carson

REU7777484

Expulsion of Christophe Thivrier from the Chamber of Deputies (colour litho)

Expulsion of Christophe Thivrier from the Chamber of Deputies (colour litho)

Belon, Joseph (1862-1927)

LLM2818478

Moments of Pleasure (Alderman Wood informs the Queen that the bill is thrown out). Published by G Humphrey, 1820.

Moments of Pleasure (Alderman Wood informs the Queen that the bill is thrown out). Published by G Humphrey, 1820.

GHL35558

Expulsion (drypoint)

Expulsion (drypoint)

Sterner, Albert Edward (1863-1946)

XDM1066733

Juifs et chretiens chasses de Rome par l'ordre de l'empereur Claude (engraving)

Juifs et chretiens chasses de Rome par l'ordre de l'empereur Claude (engraving)

French School, (19th century)

LLM3625676

Prime Minister John Major reacts after bowling out Somerset Cricket captain Andy Hayhurst during a t.., 1995 (photo)

Prime Minister John Major reacts after bowling out Somerset Cricket captain Andy Hayhurst during a t.., 1995 (photo)

Dylan Martinez

REU7481383

Death in the Air, 1933 (b/w photo)

Death in the Air, 1933 (b/w photo)

Archer, Wesley David (1916-60)

PNP700842

Rowland Taylor (1510-1555), English Protestant martyr, forcibly ejected from his church. Burned in the reign of Mary I for heresy, namely for denouncing the rule of celibacy for Roman Catholic clergy, and for denouncing the doctrine of Transubstatiation.

Rowland Taylor (1510-1555), English Protestant martyr, forcibly ejected from his church. Burned in the reign of Mary I for heresy, namely for denouncing the rule of celibacy for Roman Catholic clergy, and for denouncing the doctrine of Transubstatiation.

UIG527294

Dr. Aprill, with the imperial ban, 14th October 1757 (colour litho)

Dr. Aprill, with the imperial ban, 14th October 1757 (colour litho)

Knoetel, Richard (1857-1914)

STC434374

LOS ANGELES LAKERS GARY PAYTON RIPS OFF HIS JERSEY AFTER BEING EJECTED DURING GAME AGAINST DALLAS MAVERICKS, 2003-12-12 (photo)

LOS ANGELES LAKERS GARY PAYTON RIPS OFF HIS JERSEY AFTER BEING EJECTED DURING GAME AGAINST DALLAS MAVERICKS, 2003-12-12 (photo)

Lucy Nicholson

REU8079772

The physiognomy of the suffragette'. Portraits of Mrs Dora Montefiore, Miss Adela E.M. Pankhurst and Miss Irene Miller. A group of suffragettes ejected from the House of Commons, showing Miss Miller and Miss Billington.

The physiognomy of the suffragette'. Portraits of Mrs Dora Montefiore, Miss Adela E.M. Pankhurst and Miss Irene Miller. A group of suffragettes ejected from the House of Commons, showing Miss Miller and Miss Billington.

BL3303191

Freemasons and patriotism (engraving)

Freemasons and patriotism (engraving)

French School, (19th century)

LLM3100786

Strike against the Hershey Chocolate Company. Miles Sweeney, the CIO strike leader at the Hershey Chocolate Plant, is ejected by a mob of non-striking workers and local farmers. April 7, 1937

Strike against the Hershey Chocolate Company. Miles Sweeney, the CIO strike leader at the Hershey Chocolate Plant, is ejected by a mob of non-striking workers and local farmers. April 7, 1937

EVB2924085

American Field Artillery on the Lorraine front in Beaumont, France. An ejected shell case flies through the air as a new shell is put into the breech in the same a second. World War I. Sept. 12, 1918

American Field Artillery on the Lorraine front in Beaumont, France. An ejected shell case flies through the air as a new shell is put into the breech in the same a second. World War I. Sept. 12, 1918

Unknown photographer, (20th century)

EVB2942617

US Air Force Captain Wilmer Newk Grubb is given first aid by his captors in North Vietnam. He was taken prisoner after ejecting over North Viet Nam on Jan. 26, 1966, and died in captivity 10 days later

US Air Force Captain Wilmer Newk Grubb is given first aid by his captors in North Vietnam. He was taken prisoner after ejecting over North Viet Nam on Jan. 26, 1966, and died in captivity 10 days later

EVB2941531

Vietnam: A U.S. Air Force Boeing B-52 Stratofortress dropping bombs over Vietnam. This aircraft was hit by SA-2 surface-to-air missile over North Vietnam during the 'Linebacker II' offensive on 31 December 1972 and crashed in Laos. The crew of six ejected

Vietnam: A U.S. Air Force Boeing B-52 Stratofortress dropping bombs over Vietnam. This aircraft was hit by SA-2 surface-to-air missile over North Vietnam during the 'Linebacker II' offensive on 31 December 1972 and crashed in Laos. The crew of six ejected

PFH1173890

Ghost tendrils of Enceladus - Artist view - Enceladus icy tendrils - Artist view: Artist view of the particles and grains of ice ejects from the geysers of the satellite Enceladus - Tendril-like features from Saturn's moon Enceladus are the trajectories of tiny, icy grains ejected from Enceladus 'south polar geysers

Ghost tendrils of Enceladus - Artist view - Enceladus icy tendrils - Artist view: Artist view of the particles and grains of ice ejects from the geysers of the satellite Enceladus - Tendril-like features from Saturn's moon Enceladus are the trajectories of tiny, icy grains ejected from Enceladus 'south polar geysers

Miller, Ron (b.1947)

PIX4625913

Walter Alston Ejected, 1965 (b/w photo)

Walter Alston Ejected, 1965 (b/w photo)

UIG3448704

Sakurajima volcano erupting - Japan - Sakurajima Volcanic Eruption - Japan - Sakura-Jima volcano eruption, one of the most active volcanoes on Earth. Volcanic bombs are ejected more than 1000 meters away. January 2010. Eruption of Sakura-jima, one of the most active stratovolcano on Earth. Lava bombs flying up to 1000 meters. January 2010

Sakurajima volcano erupting - Japan - Sakurajima Volcanic Eruption - Japan - Sakura-Jima volcano eruption, one of the most active volcanoes on Earth. Volcanic bombs are ejected more than 1000 meters away. January 2010. Eruption of Sakura-jima, one of the most active stratovolcano on Earth. Lava bombs flying up to 1000 meters. January 2010

Martin Rietze

PIX4676794

Baseball Player Ejected (b/w photo)

Baseball Player Ejected (b/w photo)

UIG2621016

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 and runaway star AE Aurigae - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. The Flaming Star Nebula, IC 405, surrounds the variable star AE Aurigae. AE Aurigae is normally a 5.96 magnitude star of spectral class O. The star AE Aurigae itself is very bright, young, blue, and known as a runaway star since it appears to have been ejected from the Orion Nebula region about 2.5 million years ago

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 and runaway star AE Aurigae - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. The Flaming Star Nebula, IC 405, surrounds the variable star AE Aurigae. AE Aurigae is normally a 5.96 magnitude star of spectral class O. The star AE Aurigae itself is very bright, young, blue, and known as a runaway star since it appears to have been ejected from the Orion Nebula region about 2.5 million years ago

Adam Block

PIX4621903

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second

R. Gendler

PIX4621885

Bucking Bronco Departure (b/w photo)

Bucking Bronco Departure (b/w photo)

UIG1143057

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled in October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury, and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter is eject from the Mercury Planetary Orbiter.

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled in October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury, and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere. Here, the Mercury Magnetospheric Orbiter is eject from the Mercury Planetary Orbiter.

PIX4643601

Moon Formation: Hypotheses of impact giant - Moon Formation: Giant impact hypothesis: The hypotheses of impact giant suggests that the Moon was created from material ejecteated by a collision between the young Earth and a body the size of Mars named Theia, 4.5 billion years ago - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, approximately 4.5 billion years ago

Moon Formation: Hypotheses of impact giant - Moon Formation: Giant impact hypothesis: The hypotheses of impact giant suggests that the Moon was created from material ejecteated by a collision between the young Earth and a body the size of Mars named Theia, 4.5 billion years ago - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, approximately 4.5 billion years ago

Miller, Ron (b.1947)

PIX4614839

Nebulae IC 405 and IC 410 in the Coach - Nebulae IC 405 and IC 410 in the Coach - IC 405, on the right, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. Lower left, nebula IC 410. Image composite with H - Alpha filter. Cumulated installation time: 15 hours

Nebulae IC 405 and IC 410 in the Coach - Nebulae IC 405 and IC 410 in the Coach - IC 405, on the right, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. Lower left, nebula IC 410. Image composite with H - Alpha filter. Cumulated installation time: 15 hours

R. Gendler

PIX4621856

Nebulae IC 405 and IC 410 in the Coach - Nebulae IC 405 and IC 410 in the Coach - IC 405, on the left, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. Lower right, nebula IC 410. Image obtained with a Takahashi FSQ 106 bezel through several filters

Nebulae IC 405 and IC 410 in the Coach - Nebulae IC 405 and IC 410 in the Coach - IC 405, on the left, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. Lower right, nebula IC 410. Image obtained with a Takahashi FSQ 106 bezel through several filters

E Mouquet

PIX4621905

The Sergeant at Arms (gouache on paper)

The Sergeant at Arms (gouache on paper)

Embleton, Ron (1930-88)

LAL262071

Planetary nebula NGC 1360 in the Furnace - NGC 1360, the diffuse planetary nebula in Fornax - Image obtained by Siding Spring Planetary nebulae 3.9m telescope usually have well - defined boundaries, sometimes even a shell - like structure. For reasons that are not understood, NGC 1360 defies all these conventions, yet its colour still clearly identifies it as a planetary nebula. The green hue is oxygen, excited by the hot central star, and to the north - east of the nebula is a faint red smudge, probably traces of material ejected before the star became a true planetary nebula

Planetary nebula NGC 1360 in the Furnace - NGC 1360, the diffuse planetary nebula in Fornax - Image obtained by Siding Spring Planetary nebulae 3.9m telescope usually have well - defined boundaries, sometimes even a shell - like structure. For reasons that are not understood, NGC 1360 defies all these conventions, yet its colour still clearly identifies it as a planetary nebula. The green hue is oxygen, excited by the hot central star, and to the north - east of the nebula is a faint red smudge, probably traces of material ejected before the star became a true planetary nebula

PIX4622912

Liberal Party rally disrupted by suffragettes, 1905

Liberal Party rally disrupted by suffragettes, 1905

English School, (20th century)

XJF3037858

JOHN HOWE, CHURCHMAN

JOHN HOWE, CHURCHMAN

EPL6927451

ENGLAND CAPTAIN MICHAEL VAUGHAN,(L) LOOKS HIS STUMP AFTER BOWLED OUT BY
THE BANGLADESHI BLOWER ..., 2003-10-23 (photo) — ENGLAND CAPTAIN MICHAEL VAUGHAN,(L) LOOKS HIS STUMP AFTER BOWLED OUT BY THE BANGLADESHI BLOWER ..., 2003-10-23 (photo)

ENGLAND CAPTAIN MICHAEL VAUGHAN,(L) LOOKS HIS STUMP AFTER BOWLED OUT BY THE BANGLADESHI BLOWER ..., 2003-10-23 (photo)

Jayanta Shaw

REU7808396

PALACE AFTER KERENSKY

PALACE AFTER KERENSKY

EPL6883108

Aurora Borealis, curtain aurora, Greenland

Aurora Borealis, curtain aurora, Greenland

UIG864056

Gamma Ray Burst - Artist view - Gamma Ray Burst - Artist view - Artist view of a gamma burst, a powerful and brief emission of gamma rays whose origin is linked either to the collision of two neutron stars or to the death of a hypermassive star. Gamma - ray bursts (GRBs) are powerful flashes of energetic gamma - rays lasting from less than a second to several minutes. They release a tremendous amount of energy in this short time making them the most powerful events in the Universe. They are thought to be mostly associated with the explosion of stars that collapse into black holes. In the explosion, two jets of very fast - moving material are ejected, as depicted in this artist's illustration. If a jet happens to be aimed at Earth, we see a brief but powerful gamma - ray burst

Gamma Ray Burst - Artist view - Gamma Ray Burst - Artist view - Artist view of a gamma burst, a powerful and brief emission of gamma rays whose origin is linked either to the collision of two neutron stars or to the death of a hypermassive star. Gamma - ray bursts (GRBs) are powerful flashes of energetic gamma - rays lasting from less than a second to several minutes. They release a tremendous amount of energy in this short time making them the most powerful events in the Universe. They are thought to be mostly associated with the explosion of stars that collapse into black holes. In the explosion, two jets of very fast - moving material are ejected, as depicted in this artist's illustration. If a jet happens to be aimed at Earth, we see a brief but powerful gamma - ray burst

PIX4583341

Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added

Artist's view of a fugitive star - A runaway star in the Large Magellanic cloud - The star HE0457 - 5439 is a massive star in the Grand Cloud of Magellan; it is a star escaping from this galaxy at a speed of 2.6 Million km/h Background image obtained at the observatory of La Silla in Chile; the star fleeing has been added on the image. The star HE0457 - 5439 is a massive star wich lies closer to one of the Milky Way satellite galaxies, the Large Magellanic Cloud, located 160,000 light - years away from us. This is a runaway star, moving at more than 2.6 million kilometers per hour. Astronomers find it likely for the star to have reached its present position had it been ejected from the centre of the LMC. The background image has been obtained at La Silla observatory, the star moving has been added

PIX4572713

Anti-British cartoon, withdrawal from Gallipoli, WW1

Anti-British cartoon, withdrawal from Gallipoli, WW1

EPL6927329

Simulation of an explosion in geostationary orbit - Simulation of an explosion in geostationary orbit - A satellite in geostationary orbit moves about 3 km per second. During an explosion, debris will move more slowly and remain in the initial orbit. Some fragments will move faster than others, forming a diffuse ring around the Earth. Downstairs, the debris seen two days after the explosion. What happens after an explosion in space? A geostationary satellite has a velocity of about 3 kms/second (10,000 kms/hour). The fragments are ejected with a much lower velocity and thus stay close to the initial orbit. However, some will travel a bit faster and others a bit slower. Within a few days the debris cloud will form a diffuse ring at 36,000 km altitude around the Earth. Bottom, seen two days after the explosion

Simulation of an explosion in geostationary orbit - Simulation of an explosion in geostationary orbit - A satellite in geostationary orbit moves about 3 km per second. During an explosion, debris will move more slowly and remain in the initial orbit. Some fragments will move faster than others, forming a diffuse ring around the Earth. Downstairs, the debris seen two days after the explosion. What happens after an explosion in space? A geostationary satellite has a velocity of about 3 kms/second (10,000 kms/hour). The fragments are ejected with a much lower velocity and thus stay close to the initial orbit. However, some will travel a bit faster and others a bit slower. Within a few days the debris cloud will form a diffuse ring at 36,000 km altitude around the Earth. Bottom, seen two days after the explosion

PIX4642778

Aurora Borealis or Northern Lights

Aurora Borealis or Northern Lights

UIG864097

CELTICS PIERCE LEAVES GAME AFTER BEING EJECTED, 2002-12-21 (photo)

CELTICS PIERCE LEAVES GAME AFTER BEING EJECTED, 2002-12-21 (photo)

Ron Kuntz

REU7706282

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent feature. Covering an area of approximately 150 sq km, this crater could harbour cities such as Bonn or Kiel. In contrast to the smaller craters, it shows a blanket of ejecta with flow forms surrounding the rim. The large craters were formed when loose, soft material was ejected due to impact, and the smaller ones formed due to secondary impacts, when consolidated material was ejected in a ballistic path and impacted the original crater at varying distances. Most martian water exists in the form of subsurface ice. The presence of a blanket of ejecta and outflow channels around the crater suggest that the primary impact may have penetrated the surface enough to melt a buried frozen water reservoir — Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater at the top of the picture is 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. A larger impact crater measuring 20 km in diameter is a prominent f

PIX4616151

TIMBERWOLVES MITCHELL IS EJECTED IN THE SECOND HALF, 1997-04-26 (photo)

TIMBERWOLVES MITCHELL IS EJECTED IN THE SECOND HALF, 1997-04-26 (photo)

Adrees A.

REU7849048

III Reich, Deep sea fishing, c.1939 (photo)

III Reich, Deep sea fishing, c.1939 (photo)

SZT9229883

MIRABEAU SPEAKS

MIRABEAU SPEAKS

EPL6901344

MIAMI HEAT'S ALONZO MOURNING REACTS TO BEING EJECTED, 1996-04-27 (photo)

MIAMI HEAT'S ALONZO MOURNING REACTS TO BEING EJECTED, 1996-04-27 (photo)

Sue Ogrocki

REU8028911

Supernova 1987A 4 years after - Supernova 1987A after 4 years - Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation of Dorado on February 23, 1987. 4 years later the star appears as a red dot and pulls. The elongated red 'star' marks the site of supernova 1987A in the Large Magellanic Cloud (LMC). The two blue stars that bracket the glowing ember are almost certainly in the LMC as well, but not necessarily near the supernova. They initially confused the issue of which star had exploded. The red image is the expanding remnant of a massive star and can be seen to be slightly elongated in this picture. The elongation is in the same direction as the well - known Hubble Space Telescope picture of the ellipse around the supernova and both represent the expanding shock wave from the supernova interacting with material that was ejected from the star before it exploded

Supernova 1987A 4 years after - Supernova 1987A after 4 years - Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation of Dorado on February 23, 1987. 4 years later the star appears as a red dot and pulls. The elongated red 'star' marks the site of supernova 1987A in the Large Magellanic Cloud (LMC). The two blue stars that bracket the glowing ember are almost certainly in the LMC as well, but not necessarily near the supernova. They initially confused the issue of which star had exploded. The red image is the expanding remnant of a massive star and can be seen to be slightly elongated in this picture. The elongation is in the same direction as the well - known Hubble Space Telescope picture of the ellipse around the supernova and both represent the expanding shock wave from the supernova interacting with material that was ejected from the star before it exploded

PIX4582403

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

PIX4618685

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

Nebula of the cone NGC 2264 and S star Monocerotis - NGC 2264 and S Monocerotis - Region H II located about 2600 years - light from Earth. The bright star is S Monocerotis, a star of magnitude 4.7. Image obtained by Siding Spring's 3.9m telescope. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. Some of the wispy tendrils of nebulosity are Herbig - Haro objects, jets of matter ejected from newly - formed stars still hidden within the nebula. About 250 stars have been recognised as members of NGC 2264 which is at a distance of about 2700 light years

PIX4618722

OILERS GOALIE CONKLIN MAKES A SAVE AGAINST AVALANCHE IN FIRST PERIOD, 2003-10-23 (photo)

OILERS GOALIE CONKLIN MAKES A SAVE AGAINST AVALANCHE IN FIRST PERIOD, 2003-10-23 (photo)

Gary C. Caskey

REU7790514

Unwelcome Passengers

Unwelcome Passengers

EPL6902512

Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right

Variable star Mira Ceti view in ultraviolet - Star Mira Ceti seen in ultraviolet - Ultraviolet view of the star Mira of the Whale revealing a long train of material ejected by the large red star. This trail extends over 13 years - light. Mosaic of images obtained by the Galex satellite in November and December 2006. Ultraviolet image of the star Mira taken with the Galex satellite in November and December 2006. In this image, Mira is moving from left to right. It is visible as the small white dot in the bulb shape at right. The shed material can be seen in light blue. The dots in the picture are stars and distant galaxies. The large blue dot at left is a star that is closer to us than Mira. Mira is traveling so fast (130 kilometers per second) that it's creating a bow shock, or build - up of gas, in front of it, as can be seen here at right

PIX4572330

Matilda of Germany

Matilda of Germany

EPL6992809

PAKISTAN'S YOUNIS KHAN IS BOWLED OUT DURING THE ASIAN TEST CHAMPIONSHIP
AGAINST SRI LANKA IN LAHORE, 2002-03-06 (photo) — PAKISTAN'S YOUNIS KHAN IS BOWLED OUT DURING THE ASIAN TEST CHAMPIONSHIP AGAINST SRI LANKA IN LAHORE, 2002-03-06 (photo)

PAKISTAN'S YOUNIS KHAN IS BOWLED OUT DURING THE ASIAN TEST CHAMPIONSHIP AGAINST SRI LANKA IN LAHORE, 2002-03-06 (photo)

Mohsin Raza

REU7857879

PIRATES MCCLENDON TAKES FIRST BASE AFTER BEING EJECTED, 2001-06-26 (photo)

PIRATES MCCLENDON TAKES FIRST BASE AFTER BEING EJECTED, 2001-06-26 (photo)

Jason Cohn

REU7971386

Matilda of Germany

Matilda of Germany

EPL6803508

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas

PIX4618821

Gustave Dore Bible: Jonah cast forth by the whale (engraving)

Gustave Dore Bible: Jonah cast forth by the whale (engraving)

Dore, Gustave (1832-83)

LLM5221605

May 05, 1954 - John Cobb's Racing Car Used In Demonstration Of Retractable Aircraft Brake Parachute: Early in 1951, the C.Q. Parachute Company began work on a scheme to dispense with the necessity for jettisoning an aircraft braking parachute at the end of the landing run. A stowage system was devised by which the parachute could be automatically repacked ready for the next operation. It was decided that the parachute should be stowed in a telescopic cylinder, the rear and outer part of the cylinder being arranged to slide forwards over the inner and forward part, at the same time as the canopy was ejected rearwards by a piston engergized by a large coil spring. To retract the parachute it is only necessary to switch on the electirc winch motor. The attachment strop and parachute rigging lines would then be wound on to the drum, and when this action was complete, the telescopic cylinder would automatically extend, shrouding and stowing the parachute canopy. Seeing its possibilities as a test vehicle for aircraft brake parachute, the G.Q. Parachute Company purchased the late John Cobb's record-breaking Napier Railton racing car of 450 h.p — May 05, 1954 - John Cobb's Racing Car Used In Demonstration Of Retractable Aircraft Brake Parachute: Early in 1951, the C.Q. Parachute Company began work on a scheme to dispense with the necessity for jettisoning an aircraft braking parachute at the end of the landing run. A stowage system was devised by which the parachute could be automatically repacked ready for the next operation. It was decided that the parachute should be stowed in a telescopic cylinder, the rear and outer part of the cylinder being arranged to slide forwards over the inner and forward part, at the same time as the canopy was ejected rearwards by a piston engergized by a large coil spring. To retract the parachute it is only necessary to switch on the electirc winch motor. The attachment strop and parachute rigging lines would then be wound on to the drum, and when this action was complete, the telescopic cylinder would automatically extend, shrouding and stowing the parachute canopy. Seeing its possibilities as

May 05, 1954 - John Cobb's Racing Car Used In Demonstration Of Retractable Aircraft Brake Parachute: Early in 1951, the C.Q. Parachute Company began work on a scheme to dispense with the necessity for jettisoning an aircraft braking parachute at the end of the landing run. A stowage system was devised by which the parachute could be automatically repacked ready for the next operation. It was decided that the parachute should be stowed in a telescopic cylinder, the rear and outer part of the cylinder being arranged to slide forwards over the inner and forward part, at the same time as the canopy was ejected rearwards by a piston engergized by a large coil spring. To retract the parachute it is only necessary to switch on the electirc winch motor. The attachment strop and parachute rigging lines would then be wound on to the drum, and when this action was complete, the telescopic cylinder would automatically extend, shrouding and stowing the parachute canopy. Seeing its possibilities as

ZUM4932395

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