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Astrophysical Collection (page 20)

Astrophysical wonders never cease to amaze us, reminding us of our infinitesimal place in the vastness of the universe

Background imageAstrophysical Collection: Sunspot on the setting Sun

Sunspot on the setting Sun. The single sunspot is seen towards the centre of the solar disc. Sunspots are found in the solar atmosphere

Background imageAstrophysical Collection: VY Canis Majoris

VY Canis Majoris. Combined polarised light Hubble Space Telescope (HST) and Keck Observatory image of gaseous outbursts from the red supergiant star VY Canis Majoris

Background imageAstrophysical Collection: Eta Carinae Nebula

Eta Carinae Nebula (NGC 3372), optical image. This nebula (a vast cloud of dust and gas) surrounds the variable star Eta Carinae

Background imageAstrophysical Collection: Crab nebula

Crab nebula (M1). Composite x-ray, infrared and optical image of the Crab nebula, the remnant of a supernova. In the centre of the nebula is the remains of the stars core

Background imageAstrophysical Collection: Alien gas giant planet, artwork

Alien gas giant planet, artwork
Alien gas giant planet. Artwork of a view from above a moon orbiting an alien gas giant planet (upper centre) that is orbiting very close to its parent star

Background imageAstrophysical Collection: Swan and Eagle nebulae

Swan and Eagle nebulae, optical image. These are both emisison nebulae, clouds of gas and dust glowing red as the hydrogen gas is ionised by radiation from hot young stars within them

Background imageAstrophysical Collection: Exploding white dwarf, 3D simulation

Exploding white dwarf, 3D simulation. Supercomputer model of a white dwarf star exploding 0.9 seconds after ignition. The star surface, coloured green, measures 3, 800 kilometres in diameter

Background imageAstrophysical Collection: Omega Centauri globular cluster

Omega Centauri globular cluster
Omega Centauri (NGC 5139), the largest of the globular star clusters in our galaxy, optical image. Found in the constellation of Centaurus

Background imageAstrophysical Collection: Great Orion Nebula

Great Orion Nebula. Optical image of the emission nebulae M42 (right, large) and M43 (centre left, smaller) in the constellation Orion, together making up what is known as the Great Orion Nebula

Background imageAstrophysical Collection: Earthlike alien planet, artwork

Earthlike alien planet, artwork
Earthlike alien planet. Artwork of the view from above the surface of a moon orbiting an Earthlike alien planet (upper right)

Background imageAstrophysical Collection: Supernova, 3D simulation

Supernova, 3D simulation. Supercomputer model of a supernova simulation showing the lopsided blast waves of gas resulting from the explosion

Background imageAstrophysical Collection: Supernova explosion, 3D simulation

Supernova explosion, 3D simulation
Supernova explosion. 3D supercomputer simulation of a supernova expanding 346.7 seconds after ignition. The model represents a supernova measuring around 2.4 million kilometres in diameter

Background imageAstrophysical Collection: Earthlike planet in Orion Nebula, artwork

Earthlike planet in Orion Nebula, artwork. A small moon is at upper left, and the surface of another moon is at lower left

Background imageAstrophysical Collection: Helix Nebula

Helix Nebula (NGC 7293), optical image. This is a planetary nebula, a series of shells of gas cast off by a dying star. The ejection of the stars outer layers exposes its hot core

Background imageAstrophysical Collection: Lagoon Nebula

Lagoon Nebula (M8), optical image. This nebula is an active region of star birth. It glows red as radiation from hot, newly formed stars ionises the surrounding hydrogen gas and causes it to glow

Background imageAstrophysical Collection: Magnetar star SGR 1806-20, artwork

Magnetar star SGR 1806-20, artwork
Magnetar star SGR 1806-20. Artwork showing a gamma ray burst (blue shell) from the magnetar SGR 1806-20. A magnetar is a type of neutron star with a very strong magnetic field

Background imageAstrophysical Collection: Earthlike moons of a gas giant, artwork

Earthlike moons of a gas giant, artwork
Earthlike moons of a gas giant. Artwork of three Earthlike moons (one at upper right, two more at lower left) orbiting an alien gas giant planet

Background imageAstrophysical Collection: Supernova explosion, computer simulation

Supernova explosion, computer simulation
Supernova explosion. Computer simulation showing the gas velocities of a 15 solar mass star exploding into a supernova at one second after the start of the explosion

Background imageAstrophysical Collection: Trifid Nebula

Trifid Nebula (M20, NGC 6514), optical image. Part of this nebula (cloud of gas and dust) glows red due to the ionisation of the hydrogen gas by the hot and bright stars born at its centre

Background imageAstrophysical Collection: Spiral galaxy M66, infrared image

Spiral galaxy M66, infrared image. Blue areas are mature stars, while red areas are regions of active star formation. It is thought the distorted shape of this galaxy is due to gravitational

Background imageAstrophysical Collection: Antennae galaxies, composite image

Antennae galaxies, composite image. Two galaxies (NGC 4038 and NGC 4039) are colliding here. They are 60 million light years from Earth, in the constellation of Corvus

Background imageAstrophysical Collection: Life-cycle of the Sun, artwork

Life-cycle of the Sun, artwork
Life-cycle of the Sun, computer artwork. Our Sun was created approximately 4.6 million years ago from the gravitational collapse of giant molecular cloud (GMC, left)

Background imageAstrophysical Collection: Solar flare, 1 August 2010, SDO image

Solar flare, 1 August 2010, SDO image
Solar flare, 1 August 2010, ultraviolet SDO image. This massive solar flare (white area, upper left) impacted the Earth on 3 August 2010

Background imageAstrophysical Collection: Earth and Moon space-time warp, artwork

Earth and Moon space-time warp, artwork
Earth and Moon space-time warp. Artwork of the Earth (lower left) and the Moon (upper right) on a grid representing space-time

Background imageAstrophysical Collection: Sagittarius A, X-ray image

Sagittarius A, X-ray image
Sagittarius A. Coloured X-ray image of the supermassive black hole, known as sagittarius A-star, at the centre of our galaxy the Milky Way

Background imageAstrophysical Collection: Expanding universe, artwork

Expanding universe, artwork
Expanding universe. Artwork of galaxies and chains of clusters of galaxies in an expanding universe. Matter formed after the Big Bang

Background imageAstrophysical Collection: Starbirth region, artwork

Starbirth region, artwork
Starbirth region. Artwork of a stellar nursery, with many proto-stars lighting up the interstellar gas and dust (nebula) from which the stars are forming

Background imageAstrophysical Collection: Multiverse, artwork

Multiverse, artwork
Multiverse. Conceptual computer artwork of multiple universes (spherical) making up the multiverse, also called the meta-universe or metaverse

Background imageAstrophysical Collection: Sun over dying Earth, artwork

Sun over dying Earth, artwork
Sun over dying Earth. Computer artwork of the Sun, around 5 billion years in the future, heating a dying Earth. The oceans have evaporated, leaving salt-encrusted rocks

Background imageAstrophysical Collection: Multiverse and wormholes, artwork

Multiverse and wormholes, artwork
Multiverse and wormholes. Conceptual computer artwork of multiple universes (spherical) making up the multiverse, also called the meta-universe or metaverse

Background imageAstrophysical Collection: Swift mission gamma ray burst map, 2010

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

Background imageAstrophysical Collection: Black hole and infalling matter

Black hole and infalling matter. A black hole is formed when the core of a star collapses under its own weight, increasing the strength of its gravitational field to the point where not even light

Background imageAstrophysical Collection: Pulsar, artwork

Pulsar, artwork
Pulsar, computer artwork. A pulsar (upper right), a rapidly rotating neutron star, is the collapsed super-dense core of a massive star that has blown off its outer layers in a supernova

Background imageAstrophysical Collection: Curved time, conceptual image

Curved time, conceptual image. Abstract clock imagery representing the concepts of interdimensional space travel, time travel, and curved space-time

Background imageAstrophysical Collection: Structure of Enceladus, artwork

Structure of Enceladus, artwork
Structure of Enceladus. Cutaway computer artwork showing the interior of Enceladus, the sixth largest of Saturns moons. The surface of Enceladus is thought to be a thick layer of water ice (blue)

Background imageAstrophysical Collection: Suns gravitational field, artwork

Suns gravitational field, artwork
Suns gravitational field, computer artwork

Background imageAstrophysical Collection: Cataclysmic binary stars, artwork

Cataclysmic binary stars, artwork
Cataclysmic binary stars. Computer artwork of a red dwarf (large) orbiting around a white dwarf (small). The white dwarfs powerful gravitational force is pulling atmospheric matter away from the red

Background imageAstrophysical Collection: Time travel, conceptual image

Time travel, conceptual image

Background imageAstrophysical Collection: Black hole, conceptual image

Black hole, conceptual image
Black hole, conceptual computer artwork. Black holes are regions in space where the pull of gravity exceeds the velocity of light

Background imageAstrophysical Collection: Black hole travel

Black hole travel. Spacecraft passing a black hole as it travels though space. The white area around the black hole is its accretion disc

Background imageAstrophysical Collection: Solar wind and the Earth, artwork

Solar wind and the Earth, artwork
Solar wind and the Earth. Computer artwork showing how the Earths magnetic field (white) protects it from the Suns solar wind (yellow) by deflecting the charged particles around the planet

Background imageAstrophysical Collection: Black hole research

Black hole research. Spacecraft (top) monitoring a comet that has been drawn into a black hole (bottom). The white area around the black hole is its accretion disc

Background imageAstrophysical Collection: Hawking radiation research

Hawking radiation research. Future space probe approaching a black hole to capture Hawking radiation (blue glow). A black hole is formed when the core of a star collapses under its own weight

Background imageAstrophysical Collection: Distribution of space debris over time

Distribution of space debris over time. Computer artwork showing how the distribution of space debirs has developed over time

Background imageAstrophysical Collection: Star child, conceptual image

Star child, conceptual image
MODEL RELEASED. Star child. Conceptual image of a sleeping childs face glowing with a pale light against a background of stars. This image can represent a child dreaming of travelling to the stars

Background imageAstrophysical Collection: Earths atmosphere and radiation, artwork

Earths atmosphere and radiation, artwork
Earths atmosphere and radiation. Computer artwork showing the differing absorbance of electromagnetic waves by the Earths atmosphere

Background imageAstrophysical Collection: Wormhole travel

Wormhole travel. Image showing the theoretical possibility of a spacecraft using a wormhole in space leading from one part of the Universe (upper right) to another (lower right)

Background imageAstrophysical Collection: Space-time gateway

Space-time gateway



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Astrophysical wonders never cease to amaze us, reminding us of our infinitesimal place in the vastness of the universe. Take a moment to ponder the significance of these celestial marvels. The iconic image known as "Pale Blue Dot" captured by Voyager 1 serves as a humbling reminder of Earth's minuscule size amidst the cosmic expanse. It reminds us that we are merely inhabitants on this tiny speck floating through space. In 2012, Hubble Ultra Deep Field unveiled an awe-inspiring snapshot showcasing thousands of galaxies, each containing billions of stars. This breathtaking view allows us to glimpse into the depths of time and witness the birth and death cycles occurring across countless light-years. The historic 1919 solar eclipse provided evidence supporting Einstein's theory of general relativity, forever changing our understanding of gravity and its effects on light bending around massive objects. Orion's Belt, a prominent feature in our night sky, guides stargazers towards Orion Nebula - a stellar nursery where new stars are born from swirling clouds of gas and dust. Its ethereal beauty captivates observers with its vibrant colors and intricate details. The Pillars of Creation within Eagle Nebula stand tall as colossal columns sculpted by stellar winds and intense radiation. These towering structures serve as incubators for new star formation, reminding us that even in seemingly desolate regions lies immense potential for life to emerge. Nebula Sh 2-106 presents itself like an otherworldly painting when observed through HST imagery. Its mesmerizing mixtures of gases create stunning hues that ignite curiosity about what lies beyond our own galaxy. Gas pillars within Eagle Nebula offer glimpses into cosmic nurseries where young stars form amidst turbulent surroundings. These majestic formations showcase nature's ability to shape matter into extraordinary shapes over millions or billions of years. Once again referencing the pivotal 1919 solar eclipse.