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Astrophysics Collection (page 3)

Astrophysics, the captivating realm where science and wonder intertwine, unveils the secrets of our vast universe

Background imageAstrophysics Collection: Carina Nebula features, HST image C013 / 5604

Carina Nebula features, HST image C013 / 5604
Carina Nebula features, HST image. These pillars of gas and dust within the Carina Nebula are Herbig-Haro Objects (HH 901 and HH 902)

Background imageAstrophysics Collection: XMM-Newton telescope deployment

XMM-Newton telescope deployment
XMM-Newton deployment. Artwork showing the deployment of the XMM-Newton X-ray telescope from its Ariane 5 launch vehicle. This large satellite was deployed on 10th December`1999

Background imageAstrophysics Collection: Water on Mars, conceptual image

Water on Mars, conceptual image. Computer artwork showing frozen water ice under Mars surface

Background imageAstrophysics Collection: One of the planets orbiting 70 Virginis is a super-Jupiter

One of the planets orbiting 70 Virginis is a super-Jupiter, so close to the star that it is heated to a red heat

Background imageAstrophysics Collection: IC 2177, the Seagull Nebula

IC 2177, the Seagull Nebula. IC 2177 is a bright H II region located on the border of Monoceros and Canis Major

Background imageAstrophysics Collection: Center of the Milky Way through Sagittarius and Scorpius

Center of the Milky Way through Sagittarius and Scorpius
The Milky Way in Sagittarius (bottom) and Scorpius (left and top) including the Galactic Centre area at centre frame. Along the Milky Way are numerous deep sky objects

Background imageAstrophysics Collection: Seagull Nebula, composite image

Seagull Nebula, composite image. The image combines visible data and infrared data (orange). This star formation region is around 3500 light years distant on the borders of the constellations of

Background imageAstrophysics Collection: Helix Nebula, VISTA image C023 / 0103

Helix Nebula, VISTA image C023 / 0103
Helix Nebula. Infrared image of the Helix Nebula (NGC 7293), a planetary nebula located 700 light-years from Earth. Imaged by VISTA (Visible and Infrared Survey Telescope for Astronomy)

Background imageAstrophysics Collection: Solar activity, SDO image C023 / 8088

Solar activity, SDO image C023 / 8088
Solar activity, SDO image. Coloured image of the surface of the Sun, showing one of an unusual series of eruptions that led to a series of fast puffs

Background imageAstrophysics Collection: Kepler-35 planetary system, artwork C015 / 0790

Kepler-35 planetary system, artwork C015 / 0790
Kepler-35 planet system, artwork. This Saturn-size planet orbits a binary star system (top). The larger star is similar in size to the Sun, while the smaller stars diameter is 4/5th that of the Sun

Background imageAstrophysics Collection: M22 Globular Star Cluster, Hubble image C017 / 3722

M22 Globular Star Cluster, Hubble image C017 / 3722
M14 Globular Star Cluster (NGC 6656). This globular cluster lies around 10, 400 light years from Earth in the constellation Sagittarius

Background imageAstrophysics Collection: Milky Way-Andromeda galactic collision C014 / 4726

Milky Way-Andromeda galactic collision C014 / 4726
Milky Way-Andromeda galactic collision. Artwork showing the future collision between the Milky Way Galaxy (disrupted) and the Andromeda Galaxy (spiral, lower left)

Background imageAstrophysics Collection: Super-Earth extrasolar planet, artwork C015 / 0800

Super-Earth extrasolar planet, artwork C015 / 0800
Super-Earth extrasolar planet seen from the surface of its moon, artwork. Its parent red dwarf star is at lower centre, being transited by an inner planet

Background imageAstrophysics Collection: Spiral galaxy, HST image C013 / 5098

Spiral galaxy, HST image C013 / 5098
Spiral galaxy. Hubble Space Telescope (HST) image of the spiral galaxy NGC 3982. It is located in the constellation Ursa Major, approximately 68 million light years from Earth

Background imageAstrophysics Collection: Herschels observations of galaxies

Herschels observations of galaxies. At the time of these observations, these objects were considered to be within our galaxy

Background imageAstrophysics Collection: Nebulae drawn by William Herschel, 1811 C002 / 5044

Nebulae drawn by William Herschel, 1811 C002 / 5044
Nebulae drawn by the British astronomer William Herschel (1738-1822), published in Philosophical Transactions of the Royal Society in 1811

Background imageAstrophysics Collection: Roque de los Muchachos observatory, La Palma

Roque de los Muchachos observatory, La Palma
La Palma observatory. Panoramic view of the Roque de los Muchachos Observatory on La Palma in the Canary Islands. The observatory is located on the lip of a great volcanic caldera (right)

Background imageAstrophysics Collection: Triton and Neptune

Triton and Neptune. Computer artwork of a geyser (black) erupting from Triton, the largest moon of Neptune (blue). Triton is the coldest world in the solar system

Background imageAstrophysics Collection: Total solar eclipse

Total solar eclipse
The large, shining corona of the Sun, seen during the total solar eclipse of 11 July 1991 from Baja Caifornia, Mexico. The visible corona is in fact the overlapping K-corona and F-corona

Background imageAstrophysics Collection: Halo planet

Halo planets. Artwork showing the sky of a planet in the outer halo of a galaxy (seen from far left to upper right). The planets moon is seen at centre left

Background imageAstrophysics Collection: Comparing planetary systems, artwork

Comparing planetary systems, artwork
Comparing planetary systems. Artwork comparing the sizes of the 55 Cancri (a Sun-like system, left) and the Cha 110913-773444 (upper right) planetary systems

Background imageAstrophysics Collection: Supernova remnant IC 443, composite image

Supernova remnant IC 443, composite image. This is a combination of X-ray (blue), radio (green) and optical (red) data. A supernova remnant (SNR)

Background imageAstrophysics Collection: Hubble Space Telescope in orbit, artwork

Hubble Space Telescope in orbit, artwork
Hubble Space Telescope (HST) in orbit over the Earth, artwork. The HST is an astronomical satellite in orbit around Earth

Background imageAstrophysics Collection: Globular star cluster NGC 6101

Globular star cluster NGC 6101. This globular star cluster is located in the constellation Apus. It is around 50, 000 light years from Earth, and 36, 500 light years from the galactic centre

Background imageAstrophysics Collection: Comet Lovejoy at dawn

Comet Lovejoy at dawn over the Southern Ocean. At upper right is part of the Milky Way, the band of billions of stars that is our galaxy seen from the inside

Background imageAstrophysics Collection: 18th Century astronomical diagrams

18th Century astronomical diagrams. Historical diagrams describing various 18th Century theoretical systems used to describe the motion of the planets in our solar system

Background imageAstrophysics Collection: Evolution of the Universe, artwork

Evolution of the Universe, artwork
Evolution of the Universe. Computer artwork showing the evolution of the Universe from the Big Bang (far left) 12-15 billion years ago to the present day (far right)

Background imageAstrophysics Collection: Kepler-10b exoplanet, artwork

Kepler-10b exoplanet, artwork
January 10, 2011 WASHINGTON -- NASAs Kepler mission confirmed the discovery of its first rocky planet, named Kepler-10b. Measuring 1.4 times the size of Earth

Background imageAstrophysics Collection: Donatis Comet of 1858, artwork

Donatis Comet of 1858, artwork
Comet Donati, or Donatis Comet, formally designated C/1858 L1 and 1858 VI, was a comet named after the Italian astronomer Giovanni Battista Donati who first observed it on June 2, 1858

Background imageAstrophysics Collection: Kepler Mission rocket launch

Kepler Mission rocket launch. Delta II 7925 rocket taking off to launch NASAs Kepler Mission. This mission is designed to discover Earth-like planets orbiting other stars

Background imageAstrophysics Collection: Overlapping galaxies, HST image

Overlapping galaxies, HST image
Overlapping galaxies. Hubble Space Telescope (HST) image of the overlapping galaxies known as 2MASX J00482185-2507365. The two objects are both spiral galaxies, with the outer rim of a small

Background imageAstrophysics Collection: Stephans quintet

Stephans quintet. Optical image of Stephans quintet. This group of galaxies is 300 million light years from Earth in the constellation Pegasus

Background imageAstrophysics Collection: Pleiades star cluster, infrared image

Pleiades star cluster, infrared image
Pleiades star cluster, Spitzer infrared image. These bright young stars (blue) are surrounded by interstellar gas and dust (red, orange and green)

Background imageAstrophysics Collection: Horsehead nebula

Horsehead nebula, optical image. The horsehead shape is caused by dark nebula Barnard 33 (B 33). This cloud of dust and gas obscures the light from the emission nebula IC 434 that lies behind

Background imageAstrophysics Collection: Boomerang Nebula

Boomerang Nebula, Hubble Space Telescope image. This is a bipolar reflection nebula, where gas and dust surrounding a star are shining by reflected light

Background imageAstrophysics Collection: Sir Arthur Eddington, British astronomer, physicist and mathematician (b / w photo)

Sir Arthur Eddington, British astronomer, physicist and mathematician (b / w photo)
6014962 Sir Arthur Eddington, British astronomer, physicist and mathematician (b/w photo) by English Photographer, (20th century); Private Collection; (add.info.: Sir Arthur Eddington (1882-1944)

Background imageAstrophysics Collection: Comet Lovejoy and zodiacal light in City of Rocks State Park, New Mexico

Comet Lovejoy and zodiacal light in City of Rocks State Park, New Mexico
January 16, 2015 - A scene looking west with a field stretching up to and beyond the zenith overhead, taking in the zodiacal light stretching up to the Pleiades at upper left

Background imageAstrophysics Collection: A young star surrounded by a dusty protoplanetary disk

A young star surrounded by a dusty protoplanetary disk
This artists concept shows a young star surrounded by a dusty protoplanetary disk. This disk contains the raw material that can form planets as the star system matures

Background imageAstrophysics Collection: NGC 6559 is a rich colorful tapestry of diverse nebulosity in the constellation Sagittarius

NGC 6559 is a rich colorful tapestry of diverse nebulosity in the constellation Sagittarius. The glowing red cloud known as NGC 6559 has formed from the same molecular cloud that gave rise to its

Background imageAstrophysics Collection: EINSTEIN TOWER, POTSDAM. The Einstein Tower at Potsdam, Germany, designed, 1920

EINSTEIN TOWER, POTSDAM. The Einstein Tower at Potsdam, Germany, designed, 1920, by Eric Mendelsohn

Background imageAstrophysics Collection: XMM-Newton telescope

XMM-Newton telescope. Artwork of the XMM (X-ray Multi-Mirror)-Newton X-ray telescope in orbit above the Earth. This European Space Agency (ESA)

Background imageAstrophysics Collection: Sedna, Kuiper Belt Object

Sedna, Kuiper Belt Object
Sedna. Computer artwork of Sedna, one of the largest objects in the Kuiper Belt of the outer solar system. It is a candidate for a tenth planet because it has a relatively stable orbit

Background imageAstrophysics Collection: Pleiades star cluster (M45)

Pleiades star cluster (M45), Hubble Space Telescope image

Background imageAstrophysics Collection: Primordial quasar, artwork

Primordial quasar, artwork. Quasars are large galaxies with supermassive black holes at their centres. The gas and dust falling towards the black hole glows extremely brightly

Background imageAstrophysics Collection: Supernova remnant N132D, X-ray image

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

Background imageAstrophysics Collection: Microwave map of whole sky, c1990s

Microwave map of whole sky, c1990s. A map produced from one years data from NASAs COBE (Cosmic Background Explorer) satellite

Background imageAstrophysics Collection: Very Large Array (VLA) radio antennae

Very Large Array (VLA) radio antennae
Very Large Array antennae. View of several dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico, USA

Background imageAstrophysics Collection: Cave nebulae

Cave nebulae (Sh2-155), an emission nebula complex in the constellation Cepheus. North is at top. Emission nebulae (HII regions)



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Astrophysics, the captivating realm where science and wonder intertwine, unveils the secrets of our vast universe. From the iconic "Pale Blue Dot" image captured by Voyager 1 to the mesmerizing Hubble Ultra Deep Field 2012 photograph, astrophysics continues to expand our cosmic understanding. In 1919, during a solar eclipse, Sir Arthur Eddington's groundbreaking experiment confirmed Einstein's theory of general relativity. This pivotal moment paved the way for further astronomical breakthroughs. Gazing at Orion's Belt in awe, we are reminded of its celestial beauty and significance within our night sky. The Hubble Ultra Deep Field galaxies capture our imagination as they reveal countless distant galaxies scattered across space-time. The MAP microwave background survey provided us with an unprecedented glimpse into the early universe, uncovering ancient patterns imprinted on cosmic radiation. Meanwhile, the ethereal glow of the Orion Nebula showcases stellar birth in all its splendor. Amongst these wonders lies one of nature's most breathtaking creations: The Pillars of Creation. These colossal gas and dust structures within M16 remind us that even amidst chaos, beauty emerges. Delving deeper into nebulae like Sh 2-106 through stunning images from NASA's Hubble Space Telescope leaves us awestruck by their intricate formations and vibrant colors. Witnessing gas pillars in the Eagle Nebula evokes a sense of both fragility and resilience found throughout space. Revisiting history once more brings us back to that transformative moment during a solar eclipse in 1919 when scientific theories were validated against nature itself. It was then that humanity took another step towards unraveling universal mysteries. Lastly, we encounter the Cosmic Microwave Background (CMB), an echo from nearly fourteen billion years ago when light first permeated our expanding cosmos after the Big Bang. This faint radiation holds vital clues about our origins and paints a vivid picture of how everything began.