340 Million Pixels of GigaGalaxy Zoom

Second image from GigaGalaxy Zoom. Credit: Stéphane Guisard

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Last week the GigaGalaxy Zoom project introduced an interactive 360-degree panorama of the entire night sky, and they promised more zoomable images to come. The second of three images is now available, and it is a wonderful 340-million-pixel vista of the central parts of our galactic home. Taken by Stéphane Guisard, an ESO engineer and world-renowned astrophotographer, the image shows the region spanning the sky from the constellation of Sagittarius (the Archer) to Scorpius (the Scorpion). This mosaic was assembled from 52 different sky fields made from about 1200 individual images totalling 200 hours exposure time, with the final image having a size of 24,403 x 13,973 pixels. Click on the image to get access to larger versions of the image. Jump right in and enjoy the views!

Guisard compiled this amazing mosaic from image taken at Cerro Paranal, home of ESO’s Very Large Telescope. This second image directly benefits from the quality of Paranal’s sky, one of the best on the planet. The image was obtained by observing with a 10-cm Takahashi FSQ106Ed f/3.6 telescope and a SBIG STL CCD camera, using a NJP160 mount. Images were collected through three different filters (B, V and R) and then stitched together.

The very colourful Rho Ophiuchi and Antares region features prominently to the right, as well as much darker areas, such as the Pipe and Snake Nebulae. The dusty lane of our Milky Way runs through the image, dotted with remarkable bright, reddish nebulae, such as the Lagoon and the Trifid Nebulae, as well as NGC 6357 and NGC 6334. This dark lane also hosts the very centre of our Galaxy, where a supermassive black hole is lurking.

The GigaGalaxy Zoom project was create especially for the International Year of Astronomy.

Credit: ESO

Why is Mars Red? New Study Offers Surprises

Should Mars really be black? Credit: NASA/Mars Simulation Laboratory

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Is Mars red due to rocks being rusted by the water that once flooded the red planet? And is the only explanation for the hematite found by Mars orbiters and studied by the Mars Exploration rovers is that water once was present in volumes on Mars? Not necessarily, says a new study. Research done by Dr. Jonathan Merrison at the Aarhus Mars Simulation Laboratory in Denmark shows that the red dust that covers Mars may be formed by ongoing grinding of surface rocks. Liquid water need not have played any significant role in the red dust formation process.

“Mars should really look black, between its white polar caps, because most of the rocks at mid-latitudes are basalt,” said Merrison. “For decades we assumed that the reddish regions on Mars are related to the water-rich early history of the planet and that, at least in some areas, water-bearing heavily oxidized iron minerals are present.”

Fine red dust covers Mars’s surface and is even present in Mars’s atmosphere, dominating the weather and sometimes becoming so thick that it plunges the planet into darkness. Even though dust is ubiquitous, we do not fully understand its physical, chemical and geological properties.

Merrison and his team have been working on getting accurate measurements of the composition and mineralogy of Mars in order to understand the structure and evolution of the near-surface environment and its interaction with the atmosphere, as well as in searching for potential habitats on Mars.

In their recent laboratory study, the scientists at the Mars Simulation Laboratory have pioneered a novel technique to simulate the sand transport on Mars. They hermetically sealed sand (quartz) t samples in glass flasks and mechanically “tumbled” them for several months, turning each flask ten million times. After gently tumbling pure quartz sand for seven months, almost 10% of the sand had been reduced to dust. When scientists added powdered magnetite, an iron oxide present in Martian basalt, to the flasks they were surprised to see it getting redder as the flasks were tumbled.

Colors map percentages of hematite in the surface materials in Meridiani Planum on Mars from 5 percent (aqua) to 25 percent (red). Opportunity landed within the black oval.  MER scientists say the rocks there had once been drenched in water.  Credit: NASA
Colors map percentages of hematite in the surface materials in Meridiani Planum on Mars from 5 percent (aqua) to 25 percent (red). Opportunity landed within the black oval. MER scientists say the rocks there had once been drenched in water. Credit: NASA

“Reddish-orange material deposits, which resemble mineral mantles known as desert varnish, started appearing on the tumbled flasks. Subsequent analysis of the flask material and dust has shown that the magnetite was transformed into the red mineral hematite, through a completely mechanical process without the presence of water at any stage of this process,” said Dr. Merrison.

The scientists suspect that, as the quartz sand grains are tumbled around they get quickly eroded and an alteration of minerals through contact ensues. How exactly this happens need to be further investigated through more experimental and analytical work. What is clear though is that the first experiments show that this process occurs not only in air but also in a dried carbon dioxide atmosphere, that is, in conditions that perfectly resemble those occurring on Mars. It may also imply that the reddish Martian dust is geologically recent.

Scientists worldwide, aided by new missions and improved instrumentation reaching the planet, will continue developing new improved computer models and Earth-bound simulators to try to pierce through the red planet’s mysteries.

“By simulating the conditions and developing accurate analogues of the Martian environment, we will certainly gain a deeper understanding of its dusty nature. In particular, developing better analogues of the Martian surface and atmosphere is vital in interpreting observations made on Mars by landers as well as pioneering the next generation of experiments to be flown,” said Dr Merrison.

Merrison presented his findings at the European Planetary Science Congress last week.

Source: Europlanet

Interesting Facts About Comets

The force of gravity can cause comets to rip apart.

[/caption]There are many interesting facts about comets. Some are about the different parts of the comet, others are about the effects that comets have had on humans and their behavior. This article will let you know about the different parts of the comet, the orbital habits of a comet, and the effects that comets have had on human behavior.

There are several interesting facts about comets. The first ones involve their nucleus. Comet nuclei can range from about 100 meters to more than 40 kilometers across. They are composed of rock, dust, ice, and frozen gases such as carbon monoxide, carbon dioxide, methane, and ammonia. They have been described as “dirty snowballs”, but recent observations have revealed that they have dry dusty or rocky surfaces, suggesting that the ices are hidden beneath a crust. Comet nuclei also contain a variety of organic compounds in addition to the gases already mentioned, these may include methanol, hydrogen, hydrogen cyanide, formaldehyde, ethanol, and ethane. It is also thought that they may contain more complex molecules such as long-chain hydrocarbons and amino acids. Because of their low mass, comets cannot become round under their own gravity and will have irregular shapes. Surprisingly, cometary nuclei are among the darkest objects known to exist in the solar system. They often reflect approximately 4% of the light that falls them . In comparison, asphalt reflects 7% of the light that falls on it. It is thought that complex organic compounds are the dark surface material. The very darkness of cometary surfaces allows them to absorb the heat necessary to drive their outgassing.

The most visible part of a comet is the coma. As a comet approaches the inner solar system, radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them. The streams of dust and gas form a huge, extremely tenuous atmosphere around the comet called the coma, and the force exerted on the coma by the Sun’s radiation pressure and solar wind cause an enormous tail to form, which points away from the Sun.

The coma and tail are illuminated by the Sun and may become visible from Earth when a comet passes through the inner solar system, the dust reflecting sunlight directly and the gases glowing from ionization. The streams of dust and gas each form their own distinct tail, pointing in slightly different directions. The tail of dust is left behind in the comet’s orbit in such a manner that it often forms a curved tail called the antitail. At the same time, the ion tail, made of gases, always points directly away from the Sun. This is because gas is more strongly affected by the solar wind than is dust, following magnetic field lines rather than an orbital trajectory. While the solid nucleus of comets is generally less than 50 km across, the coma may be larger than the Sun, and ion tails have been observed to extend 1 AU or more.

Most comets have elongated elliptical orbits that take them close to the Sun for a part of their orbit, and then out into the further reaches of the Solar System for the remainder. Comets are often classified according to the length of their orbital period, the longer the period the more elongated the ellipse. Short period comets are generally defined as having orbital periods of less than 200 years. They usually orbit more-or-less in the ecliptic plane in the same direction as the planets. Their orbits typically take them out to the region of the outer planets at aphelion. Short-period comets are further divided into the Jupiter family (periods less than 20 years) and Halley family (periods between 20 and 200 years).

Long-period comets have highly eccentric orbits and periods ranging from 200 years to thousands or even millions of years. Their orbits take them far beyond the outer planets at aphelia, and the plane of their orbits need not lie near the ecliptic. Single-apparition comets are similar to long-period comets, but have parabolic or hyperbolic trajectories which will cause them to permanently exit the solar system after passing the Sun once.

Comets have been instilling fear and awe into us since man first began to look toward the sky. As early as 240 B.C. the Chinese began to document the appearance of Halley’s Comet. Ancient Greeks believed that comets resembled stars with hair flowing behind them. In ancient times, before scientists discovered what exactly comets are, many people believed that comets were a curse or a harbinger of tragedy and misfortune. It was this belief that comets were a sign of a curse that led the Roman Emperor Nero to order all of his potential successors to be executed. More recently, in 1910, as the Earth passed through Halley’s Comet’s tail, businessmen took advantage of people’s fears of impending doom and sold items such as gas masks, anti-comet pills, and umbrellas to protect users from the dangers of the comet.

There are interesting articles about comets here and another one here. Here on Universe Today there is a great article that lists many of the interesting facts about the solar system. Astronomy Cast has a very good episode about the icy outer solar system where many comets originate.

Source: NASA

What Are Comets Made Of?

Artists concept of the stardust spacecraft flying throug the gas and dust from comet Wild 2. Credit: NASA/JPL

[/caption]What are comets made of? Good question! Comet nuclei are loose collections of ice, dust and small rocky particles, ranging from a few kilometers to tens of kilometers across. As a comet approaches the inner solar system, solar radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them. The streams of dust and gas form a huge, extremely tenuous atmosphere around the comet called the coma, and the force exerted on the coma by the radiation pressure of the Sun and solar wind cause a tail to form. The tail always points away from the sun.

In order to understand what are comets made of, we need to break down the three main parts of the comet: the nucleus, coma, and tail. Comet nuclei are known to range from about 100 meters to more than 40 kilometers across. They are composed of rock, dust, ice and frozen gases such as carbon monoxide, carbon dioxide, methane, and ammonia. Sometimes called dirty snowballs, recent studies have shown that the ice of a comet is covered by a crust. Comets also contain a variety of organic compounds as well as the gases already mentioned. Some of these are methanol, hydrogen cyanide, formaldehyde, ethanol, and ethane. More complex molecules such as long-chain hydrocarbons and amino acids may also be in comets. Because of their low mass, comets cannot become spherical under their own gravity, and will thus have irregular shapes.

The coma is the the nebulous envelope around the nucleus of a comet. It is formed when the comet passes close to the Sun on a highly elliptical orbit. As the comet warms, parts of it turn from solid to gas(sublimate). Larger charged dust particles are left along the comet’s orbital path while smaller charged particles are pushed away from the Sun into the comet’s tail by solar wind. This helps astronomers distinguish comets from stars because it creates a fuzzy appearance.

The tail is illuminated by the Sun and may become visible from Earth when a comet passes through the inner solar system, the dust reflecting sunlight directly and the gases glowing from ionization. The streams of dust and gas each form their own distinct tail, pointing in slightly different directions. The tail of dust is left behind in the comet’s orbit in such a manner that it often forms a curved tail called the antitail. At the same time, the ion tail, made of gases, always points directly away from the Sun, as this gas is more strongly affected by the solar wind than is dust, following magnetic field lines rather than an orbital trajectory. Paralax viewing from the Earth may sometimes mean the tails appear to point in opposite direction.

Understanding the three parts of the comet is essential to know what are comets made of. Here is an article with a little more detail. Here on Universe Today there is a great article on a comet/asteroid hybrid. Astronomy Cast has another outstanding episode about solar dust.

Source: NASA

Astronaut Costume

Proposed spacesuits from Oceaneering, Inc. Image: NASA

Many children dream of going to space one day. While you cannot send them there now, you can at least let them pretend with an astronaut costume. These sites provide a variety of astronaut costumes. Many of the sites also have costumes for adults as well, along with an assortment of accessories.

Costume Express has a wide range of astronaut costumes for both children and adults. In addition to the white astronaut outfits, they also have blue and orange suits like those worn by NASA astronauts. There is even a jetpack backpack for kids.

Costume Craze offers a good selection of costumes. With a variety of styles for both children and adults, you can choose from orange and blue jumpsuits, or white and silver spacesuits.

The Space Store has one of the largest selections of apparel and space clothing. They have replica spacesuits that look like the real thing and are made to order as well as accessories to go with it. They also have plenty of sets for children at more reasonable prices. In addition to actual outfits, the store has NASA patches for sale.

Just Kids Costumes has several astronaut costumes from which to choose. The site also has costumes for toddlers.

Costume Zone offers a number of astronaut costumes for adults and children. They also have astronaut helmet and boots to complete the look.

Fantasy Toyland has different style astronaut costumes for your child.

Little Kids Stuff has everything your little astronaut needs – except maybe for a rocket. The site has costumes for infants up to adults. One of their best costumes is a fairly realistic-looking outfit that comes with the space suit, boots, a space backpack, and a space helmet.

Space Toys, in addition to selling toys, offers space apparel. Much of the clothing at this site is a step up from your normal Halloween costume. The merchandise at Space Toys is extremely realistic. The prices do match the higher quality though. The website has more merchandise for adults than most other sites, but they also have plenty for children as well.

Astronaut Space Suits offers high-end replica spacesuits to their customers.

Universe Today has articles on the spacesuit and how many men have walked on the Moon.

If you are looking for more information, check out making your own astronaut costume and Costume Express.

Astronomy Cast has an episode on spacesuits.

Gravity for Kids

Gravity of the Sun and Earth. Image credit: NASA

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What keeps us from floating off into space? Why does something I drop fall to the ground? Kids are famous for asking questions like this, which usually cause parents to mumble something about gravity or tell them they will learn it when they get older. Here are a number of resources that can answer some of those questions.

Kidipede explains what gravity is on the Earth and in the universe.

How Stuff Works has a number of experiments for kids regarding the laws of gravity.

Science Experiments  offers a simple science experiment about gravity for kids, including a video clip showing how to do the experiment.

The USGS has a simple definition of what gravity is.

This site explains that the reason things do not fall off the Earth is because of gravity.

Physics 4 Kids has information on gravity for children. It also covers the topics of planetary gravity and the Moon. Additionally, the site has other links to different resources.

Spaghetti Box Kids has an experiment that teaches kids about density and gravity. The project involves making miniature hot air balloons.

About.com offers information on Sir Isaac Newton and tells about his work regarding gravity and his three laws.

Teacher Tech has an entire lesson plan mapped out around Sir Isaac Newton. It teaches about Newton and his three laws of motion. Additionally, it has a quiz for students and two science experiments involving gravity and motion.

Science Monster makes learning about gravity fun and easy. In addition to providing easy to understand definitions of gravity and intertia, the website has a game you can play that further reinforces the concepts.

This is a video clip from NASA showing how important gravity is in our everyday lives. It also has links to other video clips from NASA. This material is rated for grades 5 through 12 according to NASA.

Kids Konnect  has links to a variety of sources related to gravity including NASA. The site also has a number of links to information about Sir Isaac Newton who is famous for his work regarding gravity.

Universe Today has articles on planets for kids and Solar System projects for kids.

If you are looking for more information, check out Kids Astronomy and Primary Games.

Astronomy Cast has an episode on gravitational waves.

Armillary Sphere

Armillary sphere with astrononomical clock Credit: Chris Bainbridge

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Despite the fact that the term “armillary sphere” sounds like a high-tech weapon or something from a science fiction movie, it is neither. An armillary sphere is an old tool that is supposed to represent the heavens. They were models of what scientists thought the heavens looked like and how they were suppose to have moved. The armillary sphere is also known as the spherical astrolabe, the armilla, or the armil. The armillary sphere is related to the astrolabe, which was a navigation tool used for determining the position of the Sun and stars and used by sailors for navigating.

The armillary sphere was invented hundreds of years ago. The identity of who created the sphere has been debated. Some credit its invention to a Greek named Eratosthenos. Others have said that the Chinese or other Greek scholars invented it. Regardless of its inventor, the armillary sphere is one of the oldest astronomical instruments in the world. In addition to its being used in the Greek world, the armillary sphere was also used throughout Asia and the Islamic Empire.

These devices were used as teaching tools and models. The models were used to show the difference between the Ptolemaic and Copernican theories of the Solar System. In the Copernican theory, the Sun is the center of our Solar System, while the Earth is the center of the Solar System according to the Ptolemaic theory. When armillary spheres were first invented, the Ptolemaic theory was still the accepted view. It was soon after armillary spheres were invented that Copernicus set forth his theory of the Sun as the center of the Solar System, although it was not widely accepted until centuries later.

The armillary sphere looks like a sphere circled by a ring and set upon a base. Armillary spheres were made with different numbers of circles arranged at various angles. Spheres with both four and nine circles have been known to exist – as well as ones with different numbers. These rings would then be adjusted in order to trace the path of the stars.

The armillary sphere also turns up in the Portugal flag, originally as a symbol for the country’s colony Brazil. The armillary sphere was widely used for navigating at sea, and exploration was heavily promoted by the Portugese royalty. In the early 1800’s, the sign was removed from the national flag when Brazil gained its independence. However, it was replaced in 1911 after Portugal became a Republic. You can still purchase armillary spheres today, although some of them are extremely expensive, especially if they are antiques.

Universe Today has articles on Solar System projects  and parallax.

If you are looking for further information, check out how to build an armillary sphere and astrolabes.

Astronomy Cast has an episode on telescopes.

Source: Wikipedia

Magnetic North Pole

The movement of Earth's north magnetic pole across the Canadian arctic, 1831--2001 (Geological Survey of Canada)
The movement of Earth's north magnetic pole across the Canadian arctic, 1831--2001 (Geological Survey of Canada)

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The Earth has a magnetic field, known as the magnetosphere, that protects our planet from the particles of the solar winds. One point of that field is known as the Magnetic North Pole. The Magnetic North Pole is not the geographic North Pole; it is actually hundreds of miles south of the geographic North Pole and north of Canada.

Hundreds of years ago, European navigators believed that the needles of compasses were attracted to some “magnetic mountain” or “island” thought to be located in the far north. Some also believed that the needles could be attracted to the Pole Star, which is part of the Ursa Minor constellation and has long been used in navigation. One English philosopher, William Gilbert, proposed that the Earth acts like a giant magnet; he also was the first person to state that the Earth’s magnetic field points vertically downward at the Magnetic North Pole. It took hundreds of years before scientists came to properly understand our planet’s magnetic field, although this is known to be correct now.

All magnets have two poles, like the “plus” and “minus” signs found on batteries. Instead of these locations being named plus and minus though, they were named the North and South Magnetic Poles. It is toward the Magnetic North Pole that your compass points not the geographic North Pole, which makes sense considering it utilizes magnets to determine direction. At the Magnetic North Pole, the magnetic fields points down vertically; in other words it has a 90° “dip” toward the Earth’s surface. The counterpart of the Magnetic North Pole is the Magnetic South Pole. Because the Earth’s magnetic field is not perfectly symmetrical, the magnetic fields are not antipodal. That means that if you draw a straight line between them, it does not pass through the Earth’s center. It is off by approximately 530 km. The North and South Magnetic Poles are also known as Magnetic Dip Poles because they “dip” at a 90° angle towards the Earth.   

The Magnetic North Pole continues to move around. According to the Geological Survey of Canada, which routinely studies the Magnetic North Pole, the pole moves as much as 40 km per year. It also moves daily. Every day, the Magnetic North Pole has an elliptical movement of approximately 80 km from the average point of its center. That means when you are using a compass, you have to be aware of the difference between magnetic north and geographic north.

Universe Today has articles on Earth’s magnetic field and modeling the Earth’s magnetic field.

For more information, check out the Magnetic North Pole and geomagnetism.

Astronomy Cast has an episode on Earth.

References:
Earth’s Inconstant Magnetic Field
Earth’s Magnetic Field and its Changes in Time

Looking Down the Eye of Typhoon Choi-Wan

Choi Wan on Sept. 17, 2009. Credit: the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua Satellite.

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Here’s a look at Typhoon Choi-Wan. This is a big storm covering a huge area, and luckily it is now weakening as it continues to move northeast over the Pacific Ocean. This image was taken on Sept. 18, 2009, by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua Satellite. Although the storm maintains its tightly wound symmetric shape, the striking clear eye is gone, unlike the image below, which was taken on Sept. 15. Now a category 3 storm, Choi-wan now has winds of about 200 kilometers per hour (125 miles per hour or 110 knots), whereas on the 15th, sustained winds were clocked at between 250 kilometers per hour (155 miles per hour or 135 knots) and 240 km/hr (150 mph or 130 knots), according to the Joint Typhoon Warning Center. The storm continues to skirt along the coast of Japan, causing huge waves, but is not expected to make landfall.

Typhoon Choi-Wan on Sept. 15. Credit:  The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite.
Typhoon Choi-Wan on Sept. 15. Credit: The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite.

Choi-wan was a Category 4 super typhoon in this image, and the eye is clearly visible. NASA satellite imagery showed that the tops of the thunderstorms are so high they reached the tropopause, the level of atmosphere between the troposphere and stratosphere. Those high thunderstorms mean very heavy rainfall for the area underneath. The cloud tops extended to the 200 millibar level in the atmosphere where temperatures are as cold or colder than -63 Fahrenheit.

Other infrared imagery also showed the large temperature contrast between the icy cloud tops in the storm against the warm waters in the Western Pacific Ocean that continue to power the storm.

What is the Fastest Jet In The World?

If you’re thinking the X-15 still holds the record for the fastest jet in the world, think again. That title is now owned by NASA’s X-43A. The unmanned aircraft hit Mach 9.6 (nearly 10 times the speed of sound) on November 16, 2004 at an altitude of 33,223 meters over the Pacific Ocean.

Of course, if you’re talking about manned flights, the X-15 with its Mach 6.72 speed is still king of the hill.

Both the X-15 and the X-43A are experimental aircrafts, designed to test new technologies and are usually associated with record-breaking feats. The X-15, for example, was specially designed to reach altitudes and speeds never achieved before.

Pilots of these planes were considered astronauts since many X-15 flights exceeded 50-mile altitudes. Many of them practically reached what is known as the Karman line a.k.a. the ‘edge of space’. That’s about 100 km above sea level.

If you’re looking for an aircraft that’s actually been put to use outside gathering experimental data, then the record holder is the SR-71 “Blackbird”. The Blackbird used to cruise at Mach 3.2 and was used primarily for reconnaissance missions.

Anyway, back to the fastest jet in the world – whether manned or unmanned.

As mentioned earlier, the X-43A, like its reputable predecessor, the X-15, is an experimental aircraft. Specifically, the the X-43 was part of the NASA Hyper-X program, a 7-yr program that cost around $230M and was launched to explore other options for space access vehicles.

At the heart of the X-43 is the scramjet or Supersonic Combustion Ramjet. You can think of it as an upgraded version of the ramjet – the kind of engine used by the SR-71. The Supersonic Combustion Ramjet basically takes in oxygen, which is needed for combustion, directly from the atmosphere. In order to create thrust, rockets mix liquid oxygen with liquid fuel.

In the usual jet plane setup, a tank of liquid oxygen has to be carried as additional load. Take that tank away, and you get a smaller, lighter plane. The added benefits are so enormous that engineers who embarked on scramjet research predicted speeds that could go up to 15 times the speed of sound.

Although the current record held by the scramjet-powered X-43A only achieved a fraction of that, Mach 9.6 is still way above what other planes have achieved.

To give you an idea how fast the fastest jet in the world is, compared to others, imagine this: there are more than 30 jets that are faster than the speed of sound and yet almost all of them have top speeds either way below or only near Mach 3. Mach 9.6 is definitely way way faster than that.

We have some articles in Universe Today that are related to this one. Here are two of them:

Related articles brought to you by NASA, here are the links:

Tired eyes? Let your ears help you learn for a change. Here are some episodes from Astronomy Cast that just might suit your taste:

Source: NASA