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A man leaning at the Cyclop's wall of ancient Baalbek in the Lebanon, 1920s
Reproduction of a survey of the RFA with other countries, Germany 1930s (b/w photo)
IKEA OESTERREICH GIBT ERGEBNIS 2000/2001 BEKANNT, 2001-08-07 (photo)
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IKEA OESTERREICH GIBT ERGEBNIS 2000/2001 BEKANNT, 2001-08-07 (photo)
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IKEA OESTERREICH GIBT ERGEBNIS 2000/2001 BEKANNT, 2001-08-07 (photo)
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Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) at the top, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great Galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years. Die Andromeda - Galaxie liegt in einer Entfernung von rund 2,5 Millionen Lichtjahren. Der Durchmesser der sichtbaren Scheibe betraegt 150.000 Lj. Zum Vergleich: unsere Milchstrasse hat einen Durchmesser von ca. 100.000 Lj. Nach neuesten Erkenntnissen enthaelt M31 etwa eine Billion Sterne, waehrend die Milchstrasse 100 bis 200 Milliarden Sterne enthaelt. The Andromeda - Galaxy ist umgeben von den beiden elliptischen Galaxien M32 und M110
RANDA UND SAMSTAG NACH EINER BILANZPRESSEKONFERENZ DER BANK
AUSTRIA-CREDITANSTALT, 2003-03-28 (photo)
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RANDA UND SAMSTAG NACH EINER BILANZPRESSEKONFERENZ DER BANK
AUSTRIA-CREDITANSTALT, 2003-03-28 (photo)
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European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons
Asteroide Vesta and other asteroides - Asteroid Vesta compared to other asteroids - Comparison of the sizes of the nine asteroides visits to date by space probes. The asteroid Vesta, with a diameter of 530 km, is the largest. This composite image shows the comparative sizes of nine asteroids. Up until now, Lutetia, with a diameter of 81 miles (130 kilometers), was the largest asteroid visited by a spacecraft, which occurred during a flyby. Vesta, which is also considered a protoplanet because it's a large body that almost became a planet, dwarfs all other small bodies in this image, with its diameter sizing up at approximately 330 miles (530 kilometers)
Measles Compared
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Comparison of Sun and Betelgeuse sizes - Size comparison: Betelgeuse and Sun - Betelgeuse star is a supergeant red star in the constellation Orion. It's one of the biggest stars known. It appears on this illustration at the scale next to the Sun (at the top). Betelgeuse is a red giant, one of the largest stars known. It forms the left shoulder of the constellation Orion. If Betelgeuse was placed at the center of our solar system, its fuzzy edge would extent out well beyond the orbit of Mars
Measles Compared
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Size Comparison: Earth and Jupiter - Jupiter and Earth compared - Comparison of the sizes of the Earth and Jupiter, the largest planet in the solar system. Diameter of Earth: 12 756.28 km Diametre of Jupiter: 142,984 km Jupiter's diameter is over ten times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh 426 pounds at Jupiter's cloud tops. Jupiter is five times further from the Sun than the Earth. Jupiter is so large that its famous Great Red Spot (actually a giant, hurricane-like storm that's at least 400 years old) would easily swallow the Earth. Jupiter spins so fast on its axis that it bulges noticeably at its equator (a day on Jupiter is about ten hours long)
The layers of the scalp compared to an onion and other studies, c.1490-93 (pen & ink and chalk on paper)
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Supernova 1987A before and after explosion - Supernova 1987A with precursor image overlaid - Image of the Supernova 1987A, obtained on March 8, 1987. The photo of the star Sanduleak - 69* 202, photographed two years ago. Images obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. The brightest star in the colour photograph is supernova 1987A, photographed with the AAT two months before it reached its maximum brightness. Superimposed in register on this image is a negative photograph of the region around the supernova copied from an AAT plate that was exposed in 1985, two years before the supernova was seen to explode. The precursor star appears to be a peculiar shape only because its image is blended with those of two other stars that happen to lie in the same line of sight. Many similar blended images can be seen in the colour photograph. However, it was soon found that the brighter of the three had exploded, and that was a star which had been previously observed and catalogued, as Sanduleak - 69* 202
Comparison of human and ape sculls
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A comparison of the legs of a man and of a horse, c.1506-10 (pen & ink with red chalk on paper)
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Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth
Strategy Versus Strength
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The Comparison (oil on canvas)
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Comparison of humans and monkeys
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HORSE-TRAMS VERSUS BUSES
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European launchers - Illustration - European launch vehicles family in 2009 - Illustration - Artist's view of the various fusees used by the European Space Agency and launches from the Guyanese Space Centre. From left to right, the Vega launcher, Soyuz - ST, Ariane 5 ES ATV and Ariane 5 ECA. Artist view of the family of launchers to be operated on behalf of ESA from the Guiana Space Center, Europe's Spaceport, in Kourou, English Guiana. From left to right: Vega, ESA's new small launcher, is designed to loft single or multiple payloads to orbits up to 1,500 km in altitude. Its reference payload capability is about 1,500 kg to a circular 500 - km - high Sun - synchronous orbit but it can also loft satellites from 300 kg to more than 2 metric tons, as well as piggyback microsatellites of less than 100 kg each. Soyuz - ST, the improved version of Russia's Soyuz workhorse launcher with a new digital avionics and a wider, Ariane 4 - type payload fairing. A new launch pad is being built in the CSG for Soyuz vehicles. Ariane 5 ES, another version of the Ariane 5E featuring a restartable version of Ariane 5G's storable propellant upper stage. One of its primary payloads is the Autonomous Transfer Vehicle (ATV) for resupply and reboost missions to the International Space Station. Ariane 5 ECA, the most powerful version of the Ariane 5E, an evolution of the generic Ariane 5 launcher with an increased propellant load in its solid booster stages and an improved capacity for the liquid oxygen tank of its cryogenic core stage to feed its new Vulcain 2 main engine. The Ariane 5 ECA was first launched on December 11, 2002. Its payload capacity to geostationary transfer orbit reaches 10 metric tons
Comparison of planets, illustration
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Comparison between cognac and absinthe
Tortoise and armadillo comparison
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Comparison of height and girth
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JWST mirror compares to the Hubble space telescope mirror - Size comparison between the JWST's mirror and HST's mirror - The 6.5-metre primary mirror of the James Webb Space Telescope (JWST), composed of 18 mirrors, compares to the primary mirror of the Hubble space telescope. The large JWST 6.5 meters (21.3 feet) mirror compared to the Hubble Space Telescope primary mirror (at left). The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014
Supernova 1987A before and after explosion - Supernova 1987A before and after the explosion - Images of the Supernova 1987A, on the left, obtained on March 8, 1987, and of the same photograph field on the right on February 5, 1984. Images obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. Sometime during 23 February 1987 a supernova exploded in the Large Magellanic Cloud (LMC), a nearby galaxy. However, the LMC is about 170,000 light years distant, so the supernova exploded 170,000 years ago. It was discovered the following day and brightened rapidly to become the first supernova to be easily visible to the unaided eye for almost 400 years. This photograph shows the field around the site of the supernova in great detail, both before the supernova exploded (right) and about 10 days afterwards, when it was still brightening
Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Titan images obtained by the Cassini probe on 21 March 2017. On the left, Titan seen in real colors. On the right, infrared image showing surface details as well as clouds in the northern hemisphere. These views were obtained with the Cassini spacecraft narrow-angle camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the natural-color view at left. The false-color view at right was made by substituting an infrared image (centered at 938 nanometers) for the red color channel. A large, bright and feathery band of summer clouds can be seen arcing across high northern latitudes in the view at right. The views were acquired at a distance of approximately 613,000 miles (986,000 kilometers) from Titan. Image scale is about 4 miles (6 kilometers) per pixel
Comparison of Sun and Big Stars Sizes - Size comparison: Sun and Big stars
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Woolly Mammoth and African Elephant - Comparison - Woolly Mammoth & African Elephant compared - An adult woolly mammoth (Mammuthus primigenius) that lived 150,000 years ago is compared to an adult African elephant (Loxodonta) today. The woolly mammoth was 3.3 metres tall to the shoulder and weighed 5 tonnes, while the African elephant was 3.3 metres tall to the shoulder and weighed 4.5 tonnes. An adult Woolly Mammoth (Mammuthus primigenius) from 150 thousand years ago is compared to a modern adult African Elephant (genus Loxodonta). The Woolly Mammoth is 11 feet tall at the shoulder and weighs 11,000 pounds, while the African Elephant is 11 feet tall at the shoulder and weighs 10,000 pounds
Comparison of the sizes of the main Saturn satellites. - Comparison of the sizes of the main Saturn satellites.
Growth pattern of different species of trees
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Comparison of Sun and small stars - Size comparison: Sun and small stars
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Comparison of the size of Saturn's main satellites
A comparison between a balanced and semibalanced rudder.
Diagram comparing thermometer scales, 1774
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Comparison of the Pope and Jesus Christ
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Comparison of embryos of Pig, Cow, Rabbit and Man (engraving)
Different types of brown dwarves - Artist's view - Different types of brown dwarves. Artwork - From left to right: brown dwarf type M, the youngest and most massive, temperature between 200 and 3000 degres Kelvin; brown dwarf type L, between 1500 and 2000 degres Kelvin; brown dwarf type T, between 1200 and 1500 degres Kelvin; brown dwarf type T but colder, from 1200 to 600 degres Kelvin; brown dwarf type still indefinite, less than 600 degres Kelvin; finally, on the right, Jupiter for size comparison. From left to right: a brown dwarf of type M (the youngest and most massive brown dwarves), a brown dwarf of type L, then a type T, another type T but colder, then another brown dwarf with a type unidentified yet which is colder, at last Jupiter for comparison
Comparison of Sun, Sirius and Red Giant Sizes - Size comparison: Sun Sirius and red giant
Size comparison: Earth and Saturn - Saturn and the Earth compared - Saturn, the second largest planet in the solar system compared to Earth. Saturn's diameter is about nine times greater than the Earth's. If you weigh 180 pounds on Earth, you would weigh only 165 pounds at Saturn's cloud tops (despite Saturn's enormous mass, its density is so low that if you were able to stand atop Saturn's clouds, you would feel a pull of gravity slightly less than what you feel on the Earth's surface). Saturn is ten times further from the Sun than the Earth. Saturn has the honor of being the second-largest planet in the Solar System, though it has only 30% the mass of its jovian better Jupiter. Like Jupiter, Saturn is blanketed by thick clouds and is believed to have no solid surface except for a relatively small, Earth-size core of rock and metals
The comparison of two different television sets
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Titanic compared to Trafalgar Square
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Otto von Bismarck compared to other chancellors
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Comparison between Earth and Venus - Earth and Venus compared - Comparison at the scale of the sizes of Earth and Venus, seen here without their atmosphere. The size of the Venus planet is roughly the same as that of the Earth. This to-scale image suggests how the Earth and Venus might appear without their atmospheres. Venus' diameter is 86% that of the Earth's. It has 82% the mass. If you weigh 180 pounds on the Earth, you would weigh 163 pounds on Venus. Venus is about three-quarters the Earth's distance from the Sun. While Venus is roughly the same size and density as the Earth, it is otherwise a very different world. Earth's surface is a varied one, with liquid water covering three quarters of its surface. Those areas not under water have been highly modified by plate tectonics, weather, and life itself. Venus on the other hand is far too hot to host liquid water. Volcanoes, massive lava flows and the occasional impact crater characterize its surface. Latest observations suggest that Venus may periodically resurface itself completely - and catastrophic - through massive, planet-wide volcanic eruptions. The last such resurfacing “” event”” appears to have occurred about 500 million years ago
Artist's view of the star Achernar and the Sun - Achernar. Artwork - Achernar is the brightest star in the constellation Eridan. It is characterized by a very high speed of rotation on itself (in 6.30 hours), so it is the most flattened star known to date. It's a supergiant B star. Bottom left, the Sun for comparison. Achernar is the brightest star of the constellation of Eridanus. It is star of type B, a supergiant star. Its rotation is extremely fast which gives it an oblate shape. Lower left is the Sun for size comparison