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Schematic diagram of a linear proton resonance accelerator.

Schematic diagram of a linear proton resonance accelerator.

UIG534324

United States, 1960s: animated electron and proton

United States, 1960s: animated electron and proton

AVE6328154

Proton, The Womans Wellness, Illustration, detail, 1922 (letterpress print)

Proton, The Womans Wellness, Illustration, detail, 1922 (letterpress print)

Dudovich, Marcello (1878-1962)

Ghigo Roli

GRL6375521

Proton rocket decolving 11/98 - Proton 11/98 rocket decolving a Proton rocket carrying the first element of the international space station, Zarya. 20/11/1998

Proton rocket decolving 11/98 - Proton 11/98 rocket decolving a Proton rocket carrying the first element of the international space station, Zarya. 20/11/1998

PIX4604817

Rutherford atomic model

Rutherford atomic model

UIG534767

Proton exchange membrane (PEM) fuel cell.

Proton exchange membrane (PEM) fuel cell.

UIG531431

Switzerland Cern, 1958 (b/w photo)

Switzerland Cern, 1958 (b/w photo)

Gassmann

KES6253846

Switzerland Cern, 1976 (b/w photo)

Switzerland Cern, 1976 (b/w photo)

Stringer (STR)

KES6253833

Switzerland Cern, 1976 (b/w photo)

Switzerland Cern, 1976 (b/w photo)

Stringer (STR)

KES6253832

John Adams, leader of the construction team of Proton Synchrotron which accelerated particles to 24 GeV, 24 November 1959 (b/w photo)

John Adams, leader of the construction team of Proton Synchrotron which accelerated particles to 24 GeV, 24 November 1959 (b/w photo)

UIS3506778

Emilio Segre (1905-1989), Italian-born American physicist won the 1959 Nobel Prize for Physics for the discovery of the antiproton, an antiparticle having the same mass as a proton but opposite in electrical charge. 1959

Emilio Segre (1905-1989), Italian-born American physicist won the 1959 Nobel Prize for Physics for the discovery of the antiproton, an antiparticle having the same mass as a proton but opposite in electrical charge. 1959

EVB2937601

Chemiosmosis in chloroplasts

Chemiosmosis in chloroplasts

UIG6374624

6 protons and 4 neutrons. 1950"

6 protons and 4 neutrons. 1950"

UIG1578810

Notes taken by Enrico Fermi

Notes taken by Enrico Fermi

MEP2336438

NUCLEAR PHYSICS 11 inch cyclotron, c 1931

NUCLEAR PHYSICS 11 inch cyclotron, c 1931

UIS5069049

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support communications — ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

ExoMars rover - Artist's view - Artist's view of the rover of the European mission ExoMars 2020. Artist's impression of the ExoMars rover and surface platform on the surface of Mars. The 2020 mission of the ExoMars programme will deliver a European rover and a Russian surface platform to the surface of Mars. A Proton rocket will be used to launch the mission, which will arrive at Mars after a nine-month journey. The rover will travel across the martian surface to search for signs of life. It will collect samples with a drill and analyse them in its onboard laboratory. ExoMars 2020 will be the first mission to combine the capability to move across the surface and to study Mars at depth. The surface platform, which is the responsibility of Roscosmos and the Space Research Institute of Russian Academy of Sciences (IKI), will remain stationary and will investigate the surface environment at the landing site. The ExoMars Trace Gas Orbiter, part of the 2016 ExoMars mission, will support comm

PIX4643733

6 protons and 4 neutrons. 1950"

6 protons and 4 neutrons. 1950"

UIG1578812

A RUSSIAN PROTON ROCKET IS LIFTED ONTO ITS LAUNCH PAD, 2000-09-01 (photo)

A RUSSIAN PROTON ROCKET IS LIFTED ONTO ITS LAUNCH PAD, 2000-09-01 (photo)

Karl Ronstrom

REU7915850

John Cockcroft and George Gamow, c 1930

John Cockcroft and George Gamow, c 1930

UIS5069091

Map of Fossil Radiation Seen by Planck - The cosmic microwave background as seen by Planck - The European Space Agency's Planck space telescope is the source of the data on the most detailed map ever drawn of the Cosmological Hyperrequency background radiation - the fossil radiation of the Big Bang. This image is based on data from the first 15 months of Planck operation. It is the first image of this mission that shows on the whole sky the oldest emission of light that bathed our young Universe when it was only 380,000 years old. The Universe was then filled with a burning magma of protons, electrons, and photons intertwining at about 2700oC. The interaction between protons and electrons that gave rise to the hydrogen atoms then released light. As a result of the expansion of the Universe, this light has been extended until today reaches hyperfrequency wavelengths equivalent to a temperature of just 2.7 degrees above the absolute zero. This hyperfrequency cosmological background radiation - CMB - exhibits tiny temperature fluctuations that correspond to regions of slightly different densities at periods near the origin and carry in them the germ of all future structures, stars and galaxies we know today. Acquired by Esa's Planck space telescope, the most detailed map ever created of the cosmic microwave background - the relic radiation from the Big Bang - was released revealing the existence of features that challenge the foundations of our current understanding of the Universe. The image is based on the initial 15.5 months of data from Planck and is the mission's first all-sky picture of the oldest light in our Universe, imprinted on the sky when it was just 380,000 years old. At that time, the young Universe was filled with a hot dense soup of interacting protons, electrons and photons at about 2700oC. When the proton — Map of Fossil Radiation Seen by Planck - The cosmic microwave background as seen by Planck - The European Space Agency's Planck space telescope is the source of the data on the most detailed map ever drawn of the Cosmological Hyperrequency background radiation - the fossil radiation of the Big Bang. This image is based on data from the first 15 months of Planck operation. It is the first image of this mission that shows on the whole sky the oldest emission of light that bathed our young Universe when it was only 380,000 years old. The Universe was then filled with a burning magma of protons, electrons, and photons intertwining at about 2700oC. The interaction between protons and electrons that gave rise to the hydrogen atoms then released light. As a result of the expansion of the Universe, this light has been extended until today reaches hyperfrequency wavelengths equivalent to a temperature of just 2.7 degrees above the absolute zero. This hyperfrequency cosmological background radia

Map of Fossil Radiation Seen by Planck - The cosmic microwave background as seen by Planck - The European Space Agency's Planck space telescope is the source of the data on the most detailed map ever drawn of the Cosmological Hyperrequency background radiation - the fossil radiation of the Big Bang. This image is based on data from the first 15 months of Planck operation. It is the first image of this mission that shows on the whole sky the oldest emission of light that bathed our young Universe when it was only 380,000 years old. The Universe was then filled with a burning magma of protons, electrons, and photons intertwining at about 2700oC. The interaction between protons and electrons that gave rise to the hydrogen atoms then released light. As a result of the expansion of the Universe, this light has been extended until today reaches hyperfrequency wavelengths equivalent to a temperature of just 2.7 degrees above the absolute zero. This hyperfrequency cosmological background radia

PIX4634328

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