High Energy Collection

ATLAS detector, CERN
ATLAS detector. Engineer standing on a platform in front of the ATLAS (a torodial LHC apparatus) detector (circular) at CERN (the European particle physics laboratory) near Geneva, Switzerland

ATLAS detector, CERN
ATLAS detector. Composite image of the ATLAS (a torodial LHC apparatus) detector (circular) at CERN (the European particle physics laboratory) near Geneva, Switzerland

Particle physics experiment, artwork
Particle physics experiment. Artwork of tracks of particles detected following a collision in a particle accelerator. In these experiments

CMS detector, CERN
CMS detector. Part of the CMS (compact muon solenoid) detector at CERN (the European particle physics laboratory) near Geneva, Switzerland

Lead ion collisions. Particle tracks from the first stable run lead ion collisions seen by the ALICE (a large ion collider experiment) detector at CERN (the European particle physics laboratory)

Particle physics experiment, artwork
Particle physics experiment. Artwork of tracks of particles detected following a collision in a particle accelerator. In these experiments

Lead ion collisions. Particle tracks from the first lead ion collisions seen by the ALICE (a large ion collider experiment) detector at CERN (the European particle physics laboratory) near Geneva

Zeta Ophiuchi bow shock, infrared image C016 / 9726
Zeta Ophiuchi bow shock. Infrared image from NASAs Spitzer Space Telescope (SST) of the bow shock in the interstellar medium caused by stellar winds from the fast-moving star Zeta Ophiuchi

Lead ion collisions. Particle tracks from the first lead ion collisions seen by the ALICE (a large ion collider experiment) detector at CERN (the European particle physics laboratory) near Geneva

Supernova remnant N132D, X-ray image
Supernova remnant N132D. Chandra X-ray Observatory (CXO) image of the supernova remnant N132D, an expanding shell of gas and dust from the explosion of a massive star

Galaxy cluster collision, X-ray image
Galaxy cluster MACS J0025.4-1222 collision. Combined Hubble Space Telescope (HST) and Chandra X-ray Observatory (CXO) image of a powerful collision of galaxy clusters

Solar eruption, SOHO image
Solar eruption. SOHO (Solar and Heliospheric Observatory) image of a huge coronal mass ejection (CME) from the Sun. The solar disc is obscured to prevent the image being over-exposed

Solar activity, SDO ultraviolet image
Solar activity, Solar Dynamics Observatory (SDO) ultraviolet image. The SDO is an Earth-orbiting spacecraft launched in 2010 by NASA and used to observe the Sun

X-ray binary system, artwork. X-ray binary star system, artwork. Material is being gravitationally drawn from a red giant star (upper left) by a black hole (lower right)

Cassiopeia A, NuSTAR X-ray image C016 / 9727
Cassiopeia A, NuSTAR X-ray image. This object is a supernova remnant, the expanding shell from a massive star that exploded as a supernova some 11, 000 years ago

Supermassive black hole, artwork C016 / 9724
Supermassive black hole. Artwork of an accretion disc of infalling material (orange) and a high-energy particle jet (blue) associated with a supermassive black hole at the centre of a galaxy

Spiral galaxy IC 342, NuSTAR X-ray image C016 / 9729
Spiral galaxy IC 342, NuSTAR X-ray image. This spiral galaxy, also known as Caldwell 5, is 7 million light years distant in the constellation of Camelopardalis

Mrk 231 galactic black hole, artwork C015 / 0792
Mrk 231 galactic black hole. Artwork of the environment around the supermassive black hole at the centre of the galaxy Markarian 231

Earths radiation belts, artwork
Earths radiation belts. Artwork of the Earth and its radiation belts protecting it from cosmic radiation and the solar wind. This protection is represented by a shield shape (blue)

Proton collision C014 / 1808
Particle tracks from a proton-proton collision seen by the ATLAS (a toroidal LHC apparatus) detector at CERN (the European particle physics laboratory) near Geneva, Switzerland

Giant solar flare, satellite image
Giant solar flare. Satellite image showing the development of a giant solar flare (bright) erupting from the surface of the Sun (centre)

Electron-positron collision
Particle tracks from an electron-positron collision seen by the L3 detector at CERN (the European particle physics laboratory) near Geneva, Switzerland

Solar flare, SDO ultraviolet image
Solar activity. Extreme ultraviolet (UV) satellite image showing a solar flare and coronal mass ejection (CME) erupting from the surface of the Sun on 2nd January 2012

Giant solar flare, UV telescope image
Giant solar flare. Ultraviolet (UV) image at 195nm wavelength, of a giant solar flare (bright, lower right) erupting from the surface of the Sun

SDO view of the Sun eclipsed by Earth. The Solar Dynamics Observatory (SDO) is an Earth-orbiting spacecraft launched in 2010 by NASA and used to observe the Sun

Cosmic rays, artwork
Cosmic rays. Artwork of high-energy particles and radiation from space (cosmic rays) impacting molecules and atoms in the Earths atmosphere

B-Z junction in DNA, molecular model. Deoxyribonucleic acid (DNA) occurs in three forms, A-DNA, B-DNA and Z-DNA. The first two are right-handed, with B-DNA being the more common form

Alien planet HD 189733b and stellar flare. Artwork of the exoplanet HD 189733b seen from its moon during a stellar flare. This Jupiter-sized planet is around 63 light years away in the constellation

Photon emission, artwork
Photon emission. Computer artwork of an atom (large sphere) emitting a photon (yellow). The atom consists of a nucleus (blue, centre), which contains neutrons and protons (not shown)

W33A protostar accretion disc, artwork C015 / 0806
W33A protostar accretion disc. Artwork of the accretion disc (yellow-orange), the outer torus (cloudy, dusty ring), and polar outflow jets (blue)

NGC 4889 galactic black hole, artwork C015 / 0801
NGC 4889 galactic black hole. Artwork of stars in an elliptical galaxy clustered around a supermassive black hole (upper right) of about 10 billion solar masses

Pulsar planetary disc, artwork
Pulsar planetary disc. Artwork of a planet (lower right) forming in the debris disc around a pulsar (centre). The pulsar is shown with polar jets of high-energy radiation and magnetic field lines

Quasar ULAS J1120+0641, artwork C015 / 0796
Quasar ULAS J1120+0641, artwork. The very hot extremely luminous quasar at centre of the image is very bright at ultraviolet wavelengths

Sun, Earth and solar flare, artwork C013 / 9496
Sun, Earth and solar flare, artwork. Solar flares are eruptions in the solar atmosphere that cause a large increase in levels of dangerous radiation and charged particles

Swift mission gamma ray burst map, 2010
Swift mission gamma ray burst map. This map shows the 500 gamma ray bursts (GRBs) detected by NASAs Swift mission while in Earth orbit between December 2004 and April 2010

Gravity waves in space-time, artwork. Space-time, the treatment of space and time as a unified whole, was developed by Einstein in his theories of Relativity

Particle collision, artwork

Earth and gravity waves, artwork
Earth and gravity waves. Artwork showing the Earth above a set of gravity waves, set against a starry background. Gravity waves are fluctuations in the curvature of space-time which propagate as a

Abell 1689 galaxy cluster, X-ray image
Abell 1689 galaxy cluster. Combined Hubble Space Telescope (HST) and Chandra X-ray Observatory (CXO) image of the massive galaxy cluster Abell 1689

Supernova remnant SN1006, composite image
Supernova remnant SN 1006. Combined X-ray, radio and optical image of the supernova remnant SN 1006, an expanding shell of gas and dust from the explosion of a massive star

Supersymmetric particle production. Computer artwork showing the results of a collision between a quark (pink) and an antiquark (blue)

Cyclotron particle accelerator being examined by scientists and technicians. This is a U-400 cyclotron at Russias United Institute for Nuclear Research

Linear particle accelerator. This is one end of a linear (straight) particle accelerator. Linear particle accelerators accelerate particles in a straight line

First photo of ultraheavy primary cosmic ray
First picture of an ultraheavy cosmic ray primary, compared with a cosmic ray iron nucleus. The tracks of both nuclei are recorded in photographic emulsion exposed during balloon flights high in

Synchrotron particle accelerator. The hole in the floor shows someone examining the circular tube within which particle beams are accelerated to high energies

HEGRA gamma ray telescope
Gamma ray telescope. Cerenkov telescope at the High-Energy-Gamma-Ray Astronomy (HEGRA) site at the Roque de los Muchachos Observatory on La Palma, Canary Islands

LHC tunnel, CERN
LHC tunnel, composite image. Safety supervisor riding a bicycle along the LHC (large hadron collider) tunnel at CERN (the European particle physics laboratory) near Geneva, Switzerland

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"Unleashing the Power of High Energy: Exploring the Mysteries of the Universe at CERN" Step into the world physics, where groundbreaking experiments and mind-boggling collisions take place. At CERN, home to cutting-edge scientific research, two remarkable detectors stand tall - ATLAS and CMS. These colossal machines are at the forefront of unraveling the secrets hidden within particles. In this captivating artwork, a particle physics experiment comes alive as vibrant colors dance across the canvas. It symbolizes our relentless pursuit to understand nature's building blocks and their intricate interactions. Witness an extraordinary phenomenon - lead ion collisions. As these tiny particles collide with tremendous force in accelerators like LHC, they create conditions akin to those moments after the Big Bang. Scientists delve into this cosmic chaos to unlock fundamental truths about our universe's origins. Gaze upon Zeta Ophiuchi bow shock captured through an infrared lens - a mesmerizing display of energy unleashed by a massive star hurtling through space. This celestial spectacle reminds us that high energy phenomena exist not only on Earth but also throughout our vast cosmos. Behold Supernova remnant N132D in its X-ray glory. The remnants left behind by exploding stars emit intense radiation, providing invaluable insights into stellar evolution and cataclysmic events that shape galaxies. Venture deep underground into the labyrinthine tunnels housing LHC - a technological marvel spanning kilometers beneath CERN's surface. Within these tunnels lies humanity's quest for knowledge; where scientists push boundaries using unimaginable energies to explore uncharted territories. Marvel at galaxy cluster collision imprinted in X-ray brilliance. Witnessing such immense forces colliding is like witnessing nature's grandest fireworks display – illuminating dark matter mysteries while shaping galactic landscapes. High energy science takes us beyond what we can see with naked eyes; it propels us towards understanding existence itself.