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Astrophysical Collection (page 26)

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

Background imageAstrophysical Collection: TRACE observatory

TRACE observatory over Earth, computer artwork. TRACE (Transition Region and Coronal Explorer) is a space observatory launched in 1998 to study the Sun at ultraviolet wavelengths

Background imageAstrophysical Collection: TRACE observatory, artwork

TRACE observatory, artwork
TRACE observatory, computer artwork. TRACE (Transition Region and Coronal Explorer) is a space observatory launched in 1998 to study the Sun at ultraviolet wavelengths

Background imageAstrophysical Collection: TRACE observatory and the Sun, artwork

TRACE observatory and the Sun, artwork
Solar coronal loops. Computer artwork based on the ultraviolet TRACE image of the Sun, showing coronal loops following a solar flare event observed in November 2000

Background imageAstrophysical Collection: TRACE observatory and solar coronal loops

TRACE observatory and solar coronal loops
Solar coronal loops. Computer artwork based on the ultraviolet TRACE image of the Sun, showing coronal loops following a solar flare event observed in November 2000

Background imageAstrophysical Collection: Alien planets and space warp, artwork

Alien planets and space warp, artwork
Alien planets and space warp, computer artwork. Several extrasolar planets and moons are seen here, against a background of stars. Three planets or moons are at upper right, and one is at bottom

Background imageAstrophysical Collection: Moon and stars, artwork

Moon and stars, artwork
Moon and stars, computer artwork. The Moon is a heavily cratered, barren, airless and rocky astronomical body that orbits the Earth (not seen) at a distance of 385, 000 kilometres

Background imageAstrophysical Collection: Betelgeuse emission spectrum

Betelgeuse emission spectrum
Sirius emission spectrum. This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitted by the star Betelgeuse (Alpha Canis Majoris)

Background imageAstrophysical Collection: Omicron Ceti emission spectrum

Omicron Ceti emission spectrum. This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitted by the star Omicron Ceti (Mira Ceti)

Background imageAstrophysical Collection: Pleiades emission spectra

Pleiades emission spectra. These multicoloured bands are obtained by recording what wavelengths of light (each seen as a different colour) are emitted by each star in the open cluster Pleiades

Background imageAstrophysical Collection: Cosmic man juggling worlds, artwork

Cosmic man juggling worlds, artwork
Cosmic man juggling worlds. Conceptual computer artwork of a figure illuminated by polarised light, standing on the Earth and juggling four globes. The background is a starry night sky

Background imageAstrophysical Collection: Total solar eclipse, artwork

Total solar eclipse, artwork
Total solar eclipse. Computer artwork of the stages before and after a total solar eclipse (centre). The outer corona (white) is seen here

Background imageAstrophysical Collection: HEGRA gamma ray telescope

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

Background imageAstrophysical Collection: Watching solar eclipse

Watching solar eclipse. Young boy using special protective viewing glasses to observe a solar eclipse (upper right). They are designed to block most of the light from the Sun

Background imageAstrophysical Collection: Mars as seen from Phobos, artwork

Mars as seen from Phobos, artwork
Mars as seen from Phobos, computer artwork. Phobos (grey, foreground) is the larger of the two Martian moons. It is irregular in shape, measuring 19 by 21 by 27 kilometres

Background imageAstrophysical Collection: Total solar eclipse, artwork

Total solar eclipse, artwork
Total solar eclipse. Computer artwork of the outer corona of the Sun, seen during a total solar eclipse. The corona is the cloud of low-density plasma (hot ions) that surrounds the Sun

Background imageAstrophysical Collection: Schiaparelli crater, Mars, artwork

Schiaparelli crater, Mars, artwork
Schiaparelli crater, Mars. Computer artwork of the impact crater (upper centre) named after the Italian astronomer Giovanni Schiaparelli (1835-1910)

Background imageAstrophysical Collection: Christmas Tree Cluster (NGC 2264)

Christmas Tree Cluster (NGC 2264)
Christmas Tree cluster (NGC 2264), optical image. This nebula, also known as the Cone Mosaic nebula, consists of clouds of dust

Background imageAstrophysical Collection: Open star cluster M11

Open star cluster M11. It is also known as the Wild Duck cluster. *** THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY NOAO ENDORSEMENT OF ANY COMPANY OR PRODUCT ***

Background imageAstrophysical Collection: Fornax A galaxy

Fornax A galaxy. Combined optical (white) and radio (orange) image of the galaxy Fornax A (NGC 1316, centre). The smaller galaxy NGC 1317 is above it

Background imageAstrophysical Collection: Ring nebula (M57)

Ring nebula (M57)
Ring Nebula (M57). *** this Picture May Not be Used to State or Imply Noao Endorsement of any Company or Product ***

Background imageAstrophysical Collection: Tarantula nebula

Tarantula nebula. The tarantula nebula, also known as 30 Doradus, is found in the Large Magellanic Cloud, approximately 170, 000 light years from Earth

Background imageAstrophysical Collection: Moon in transit across Sun

Moon in transit across Sun. Image 2 of 3. Transit of the Moon across the Sun, as seen from the Stereo-B spacecraft. This event was not visible from Earth

Background imageAstrophysical Collection: Saturns moon Tethys, Cassini image

Saturns moon Tethys, Cassini image
Saturns moon Tethys. False-coloured Cassini image of Tethys, one of the moons of Saturn. This is the side of Tethys that faces away from Saturn

Background imageAstrophysical Collection: Saturn, Cassini infrared image

Saturn, Cassini infrared image. This view is of a region of Saturns northern hemisphere. A section of the rings (blue) is visible at upper left

Background imageAstrophysical Collection: Young star cluster, artwork

Young star cluster, artwork
Young star cluster. Artwork of a young star cluster seen from near a planet (lower right, green) orbiting the brightest star (centre right)

Background imageAstrophysical Collection: Rosette Nebula, infrared image

Rosette Nebula, infrared image. This area of the nebula (a large cloud of gas and dust) shows a cavity formed by the strong stellar winds of a hot type of star called O-stars

Background imageAstrophysical Collection: Cistus x argenteus Silver Pink flower

Cistus x argenteus Silver Pink flower
Rock rose flower (Cistus x argenteus Silver Pink )



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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.