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Nutmeg (Myristica fragrans) 2004 (w/c on paper)
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The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide
Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory
Core of a Comet - Illustration - Comet nucleus Artwork
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Cross-section view of the Earth - Earth cutaway - Internal structure of the Earth. On the surface, the crust forms a bark of about 7 km under the oceans and 30 to 40 km under the continents. Below is the mantle, a 2900 km thick rock belt. The outer core is composed of liquid metal, mainly iron and nickel. The inner core, or seed, is composed of the same alloy but is solid. Art cutaway of Earth showing interior structure. The surface is a crust, a thin layer of solid rock about 7 km thick under the oceans and 30 to 40 km thick where there are continents. Below is the mantle, 2900 km thick layer of molten rock. The outer core consists of liquid metal, mostly iron and nickel. The inner core has a similar composition but is solid
The stages of Earth formation - Artist view - Earth formation - Artist view - The Earth was formed 4.5 billion years ago from a gigantic cloud of gas and dust. From microscopic grains, planetesimal form, clash and agglomerate to form our planet; it was then subjected to a large bombardment of meteorites bringing a significant share of the water to Earth. Earth formed 4.54 billion years ago from a large protoplanetary disk accreting. The proto earth was bombarded by planetoids heating the newly formed planet
The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (back view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory
Nutmeg and mace tree, Myristica moschata, Myristica fragrans
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Nuts and Filberts (top to bottom, left to right): common white filbert; scarlet fillbert; Barcelona filbert; English cob nut and varieties; white and brown hazelnuts from 'Pomona Britanica', 1812 by George Brookshaw
Core of Comet 67P/Churyumov - Gerasimenkovu by the Rosetta probe - Comet 67P/Churyumov - Gerasimenko nucleus seen by Rosetta - Image of the nucleus of Comet 67P/Churyumov - Gerasimenko seen on November 22, 2014 by the Rosetta probe at a distance of 30 km. OSIRIS wide - angle camera image acquired on 22 November 2014 from a distance of 30 km from Comet 67P/Churyumov - Gerasimenko. The image resolution is 2.8 m/pixel. The nucleus is deliberately overexposed in order to reveal the faint jets of activity
Surface of a comet - Illustration - Comet surface - Illustration
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Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Composite of images of the nucleus of the Hartley 2 comet obtained on November 4, 2010 during its approach by the Epoxi probe (Deep Impact). The core is 2 km long. This image montage shows comet Hartley 2 as NASA'S EPOXI mission approached and flew under the comet. The images progress in time clockwise, starting at the top left. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus
Core of Comet Wild 2 - Comet Wild 2 nucleus - The nucleus of Comet Wild 2 (5 km in diameter) seen by the Stardust probe on January 2, 2004. This image was taken during the close approach phase of Stardust's Jan 2, 2004 flyby of comet Wild 2. It is a distant side view of the roughly spherical comet nucleus. One hemisphere is in sunlight and the other is in shadow analogous to a view of the quarter moon. Several large depressed regions can be seen. Comet Wild 2 is about five kilometers (3.1 miles) in diameter
Core of the Tempel 1 comet seen by the Deep impact probe - Comet Tempel 1 nucleus seen by Deep impact spacecraft - Composite image of different cliches. The core is 5 km by 7 km. This composite image was built up from scaling all images to 5 meters/pixel, and aligning images to fixed points. Each image at closer range, replaced equivalent locations observed at a greater distance. The impact site has the highest resolution because images were acquired until about 4 sec from impact or a few meters from the surface
Core of Comete Hale - Bopp 03/04/1997 - Comet Hale - Bopp nucleus - Comet Hale - Bopp nucleus. April 3 199
A comete breaks - Illustration - Comet breaking up
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Comet 67P/Churyumov-Gerasimenko nucleus seen by Rosetta probe - Comet 67P/Churyumov-Gerasimenko nucleus seen by Rosetta: Editing 18 images showing the activity of Comet 67P/Churyumov-Gerasimenko between January 31, 2015 (top left) and March 25, 2015 (bottom right) when the Rosetta probe was a distance between 30 and 100 km from the centre de la comete - This spectacular montage of 18 images shows off the comet's activity from many different angles as seen between 31 January (top left) and 25 March (bottom right), when the spacecraft was at distances of about 30 to 100 km from the comet. At the same time, Comet 67P/Churyumov-Gerasimenko was at distances between 363 million and 300 million km from the Sun
Core of comet 67P/Churyumov-Gerasimenko seen by Rosetta - Comet 67P/Churyumov-Gerasimenko nucleus from Rosetta: Image of the surface of comet 67P/Churyumov-Gerasimenko taken at an altitude of 16 km during the final descent of the Rosetta probe on 30 September 2016. Rosetta's OSIRIS narrow-angle camera captured this image of Comet 67P/Churyumov-Gerasimenko at 01:20 GMT from an altitude of about 16 km above the surface during the spacecraft's final descent on 30 September. The image scale is about 30 cm/pixel and the image measures about 614 m across
Core of the Hartley 2 comet seen by the Epoxi probe - Comet Hartley 2 nucleus seen by Deep impact spacecraft - Image of the core of the Hartley 2 comet seen on November 4, 2010 by the probe Epoxi (Deep Impact) at a distance of 700 km. The core is 2 km long. The image, one of the closest taken of comet Hartley 2 by NASA'S EPOXI mission, shows many features across the comet's surface. There are two obvious regions of jet activity associated with rough terrain. The smooth surface in the middle is lower than the rest of the comet and may accumulate fine - grain dust. The image was taken by Epoxi's Medium - Resolution Instrument on Nov. 4, 2010. The sun is to the right. The comet's nucleus, or main body, is approximately 2 kilometers (1.2 miles) long and 0.4 kilometers (0.25 miles) at the “” neck,””” or most narrow portion. Jets can be seen streaming out of the nucleus
Core of Comet Tempel 1 - Illustration - Tempel 1 comet nucleus.
Surface of a comet - Illustration - Comet surface - Illustration: Away Earth and Moon
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Core of a Comet - Illustration - Comet nucleus. Artwor
Stardust probe and comet Wild 2 - Artist view - The Stardust probe and comet Wild 2 - Artist view - The Stardust probe was launched on February 7, 1999 with the primary objective of studying the comet Wild 2 and taking samples during a passage through the comet's hair. Stardust was the first probe to collect and bring back to Earth interstellar and cometary dust. The return capsule landed on Earth on 15 January 2006 with the samples. Stardust is an interplanetary spacecraft, whose primary purpose was to investigate the makeup of the comet Wild 2 and its coma. It was launched on February 07 1999 and returned to Earth on January 15 2006. It is the first sample return mission to collect cosmic dust and return the sample to Earth; the capsule contains cometary and interstellar samples gathered by the Stardust spacecraft
Comet 67P/Churyumov-Gerasimenko and Philae - Comet 67P/Churyumov-Gerasimenko nucleus with Philae: Detail of the surface of the nucleus of Comet 67P/Churyumov-Gerasimenko as seen on September 2, 2016 by the Rosetta probe. The Philae lander appears pose on the comet - Rosetta's lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel - Philae's 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae's orientation - A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked
Galaxy NGC 660 in Pisces - Galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image of the central part of the galaxy obtained by the Hubble Space Telescope (HST). NGC 660 is described as being a “” polar ring””” galaxy. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million light years away. Image taken with the Hubble space telescope (HST)
Center of the Andromede Galaxy (M31) - Central part of the Andromeda galaxy (M31) - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained with a telescope measuring 61 centimetres in diameter shows the central region of the galaxy where a huge mass of stars is orbiting around the nucleus. The central part of M31 where the huge mass of stars are in orbit around its nucleus. Image taken with a 24 - inch telescope on october 13 2009
Core of a Comet - Illustration - Comet nucleus. Artwork - View of comet artist in the cloud of Oort
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Comete et planete giant - Comet approaching a giant planet - Comet approaching a giant planet. Breakup of a comet nucleus approaching a giant planet. Artwork
Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the central region of the galaxy where a huge mass of stars is orbiting around the nucleus. This picture covers almost half a degree of sky (about the size of the full moon), but wide angle telescopes show the galaxy to be over three degrees long at its widest. Here we see only the central part of M31, the huge mass of stars that are in orbit around its nucleus. Silhouetted against this starry background are tangled sheets and curtains of dust, very reminiscent of dust clouds we see in our own galaxy. This picture was made from three black and white glass negatives. Some care has been taken to ensure that the colours seen here are realistic
Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of M31 there lurks a black hole, accelerating stars close to it to abnormally high velocities. Similar effects are seen in the Milky Way, but in our galaxy the nucleus is hidden at optical wavelengths, so observations are made in the infrared and at radio wavelengths
A comet approaches the Sun - Illustration - Comet near our Sun - artwork - Artwork of a comet approaching our sun
Nuclei of the 5 cometes visited by probes - 5 Comets nucleus seen by spacecrafts - Comparison of the size of the nuclei of the five comets visited by space probes. This montage shows the only five comets imaged up close with spacecraft. The comets vary in shape and size. Comet Hartley 2 is by far the smallest and the most active of small comets. This jet activity can be seen extending from the comet's surface and into its outer shell of gas and dust, or coma. This is first time scientists have been able to link jets to the details of the surface
The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (front view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory
Le Soleil vu en coupe - Sun cutaway - Cutaway of the sun
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Rosetta probe: the lander is dropped on the core of the comet - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on March 2, 2004 to study comet 67P/Churyumov - Gerasimenko. Artist view of the probe and lander Philae near the core of the comet. The size scales are not respected, the probe measures 32 metres with its deployed panels, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide
Le Soleil vu en coupe - Sun cutaway - Cutaway of the sun
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Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory
The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected; the probe measures 32 meters with its deployed panels; the core of the comet about 4 km.; Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko.; The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays; while the comet nucleus is thought to be about 4 km wide
Three cobs of corn showing variations in colour, caused by transposon segments of DNA
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Bowl containing bones, nuts and shells, South African, 1890-1924
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Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) on the left and M110 (NGC 205) (off-field). Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. The several distinct stars that surround Andromeda's image are actually stars in our Galaxy that are well in front of the background object. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei
Spiral Galaxy M83 in Hydra - M83 (NGC 5236) - The galaxy M83 (NGC 5236) is about 15 million light years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Composite images obtained from the Hubble Space Telescope (HST), the Subaru Telescope and the 2.2m MPG telescope of the ESO. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Composite image from four data sources (8.2 Meter Subaru Telescope, Hubble Space Telescope, 2.2 - meter Max Planck - ESO telescope and 14.5” RC)
Core of the Andromede Galaxy (M31) - The Andromede Galaxy is located about 2 million years away - light from Earth. View of its dual nucleus obtained by the Hubble Space Telescope (HST). Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei. Image taken with the Hubble space telescope (HST)
Core of the spiral galaxy NGC 300 in the Sculptor - Nucleus of galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. This photo made by the Hubble Space Telescope in 2006 shows the central part of the galaxy where a brilliant cluster of stars appears near the core of the galaxy. NGC 300 resides 7 million light - years from Earth. In this image, Hubble space telescope resolves a dense swarm of stars, patches of dust, and a bright central star cluster. This cluster lies at the very nucleus of the galaxy. Similar clusters are thought to be related to the formation of supermassive black holes. NGC 300 is part of a detailed survey called the ACS Nearby Galaxy Survey Treasury program (ANGST). In this census Hubble observed roughly 14 million stars in 69 galaxies
Central region of the spiral galaxy NGC 300 in the Sculptor - Nucleus of spiral galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. The photo taken by Siding Spring's 3.9m telescope highlights the nucleus of this galaxy. At the centre of the spiral arms of NGC 300 is an unusually compact, star - like nucleus. It is surrounded by a faint but extensive yellow haze, consisting of millions of faint, cool stars. This is the older population, or 'bulge' of NGC 300, a distant equivalent to the (much more numerous) stars that we see in our own galaxy as the brightest part of the Milky Way in Sagittarius
Galaxy M83 in Hydra - Galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is about 15 million years away from Earth. This galaxy is a barred spiral. Image obtained by the Hubble Space Telescope (HST). M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The vibrant magentas and blues reveal the galaxy is ablaze with star formation. This photograph captures thousands of star clusters, hundreds of thousands of individual stars, and “” ghosts”” of dead stars called supernova remnants. The galactic panorama unveils a tapestry of the drama of stellar birth and death spread across 50,000 light - years.Image taken with the Hubble space telescope (HST)
Threshing machine. K series. Engraving by Haure, 1870.
Nutmeg and mace tree, Myristica moschata, Myristica fragrans, from a botanical illustration by James Sowerby from William Woodville and Sir William Jackson Hooker's "Medical Botany" 1832 (handcoloured copperplate engraving)
Exploring a Comet - Illustration - Exploring a Comet - Illustration: Astronauts Exploring a Comet
Threshing machine. H series. Engraving by Haure, 1870.
United States 1950s: A researcher removes a bag from the top of a cornstalk, collecting the kernels as he does so
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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth
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Green and red seeds of nutmeg and mace, Myristica fragrans Houtt.
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Green and pink seeds of nutmeg and mace, Myristica fragrans Houtt.
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Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth
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Indian corn in a row
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Comet nucleus and planet - Illustration - Comet nucleus and a planet Artwor
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African oil palm tree with fruit, Elaeis guineensis
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The first galaxies - The first galaxies - Artist's view of the appearance of giant stars at the intersection of hydrogen filaments, which will form the nuclei of the first galaxies. Giant stars form at the intersections of great filaments of primordial hydrogen, forming the nuclei of the first galaxies
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Le Soleil vu en coupe - Sun cutaway: Cutaway of the sun, showing core, radiative and convective zones, and corona
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A laser shot attempts to deflect a comet nucleus - Illustration - High - powered laser to deflect a comet nucleus - Illustration - A powerful laser pulls from Earth's orbit, tries to deflect a threatening comet. A high - powered laser in earth orbit blasts surface material from an approaching comet nucleus in an effort to deflect it
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Chilean Stirfry in a Wok (photo)
Kernel (coconut") of the fruit of the Cocos nucifera,
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Biscuit with currants, pine kernel and walnut, Italy
Biscuit with currants, pine kernel and walnut, Italy
Euterpe edulis/Palm tree/Palm kernel jucara
Croquette of vegetables on boiled vegetables and pine-kernel, Italy
Croquette of vegetables on boiled vegetables and pine-kernel, Italy