Scientist Says Texting is More Expensive Than Downloading From Hubble

Does your cell phone bill ever reach astronomical proportions? Maybe you’re doing too much texting. One space scientist has worked out that sending texts via mobile phones works out to be far more expensive than downloading data from the Hubble Space Telescope. Dr. Nigel Bannister from the University of Leicester looked at the cost of obtaining a megabyte of data from Hubble and compared it with the cost of sending a text. His calculations? “The bottom line is texting is at least 4 times more expensive than transmitting data from Hubble, and is likely to be substantially more than that.”

Bannister says, “The maximum size for a text message is 160 characters, which takes 140 bytes because there are only 7 bits per character in the text messaging system, and we assume the average price for a text message is 5 pence (about .10 USD). There are 1,048,576 bytes in a megabyte, so that’s 1 million/140 = 7490 text messages to transmit one megabyte. At 5p each, that’s £374.49 ($734.25 USD) per MB – or about 4.4 times more expensive than the ‘most pessimistic’ estimate for Hubble Space Telescope transmission costs.”

Dr Bannister said NASA provided the numbers of £8.85 ($17.33 USD) per megabyte for the transmission of data from HST to the Earth.

“This doesn’t include the cost of the ground stations and the time of the personnel along the way, but it is an unambiguous number for that part of the process. So that’s £8.85 to get each MB from Hubble, to the first point of contact on the ground, but no further. Hence we need to go a little bit further to estimate exactly how much it costs to transmit data from Hubble to the end user – i.e. to the data archive which scientists can access. This is difficult, so I had to make some conservative assumptions.”

Dr. Bannister estimated the cost of the data from Hubble could vary between £8.85 and £85 per MB- much cheaper than the £374.49 per MB cost of transmitting one MB of text.

Surprised by the results, Bannister said, “Hubble is by no means a cheap mission – but the mobile phone text costs were pretty astronomical!”

Original News Source: Physorg.com

Hubble Image of the Colliding Antennae Galaxies (with Video)

Antennae Galaxies. Image credit: Hubble

It’s time for another beautiful image from the Hubble Space Telescope. And this time, there’s an added bonus… video. The latest images released by Hubble are based on research of the Antennae Galaxies, known as NGC 4038 and NGC 4039. Astronomers used to think that they were 65 million light-years away, but the new research puts them much closer; probably 45 million light-years away.

This image was captured by Hubble’s Advanced Camera for Surveys and Wide Field Planetary Camera 2, to observe individual stars spawned by the cosmic collision.

Here’s the Hubble video to help you get a sense of the scales involved (with pretty music too).

The astronomers targeted the object’s southern tidal tail, which was thrown away from the active central regions. This tail contains material hurled away from the main galaxies as they came together. Astronomers looked for older red giants to make the estimate for their distance. These red giants are known to always shine with the same brightness, and by knowing this brightness, they were able to calculate the galaxies as being 45 million light-years away.

Since this galactic merger is happening relatively close, it’s one of the best examples astronomers have to study this process. And now that the galaxies are closer than astronomers previously believed, it changes the size of many objects the astronomers are studying. For example, the size of the star clusters being formed by the collision match the size of other galaxy mergers, instead of being 1.5 times larger than they should be.

The Antennae Galaxies are named for the two long tails of stars, gas and dust thrown out of the collision that resemble the antennae of insects. They can be found in the constellation of Corvus, the Crow.

Original Source: Hubble News Release

Hubble Surprise: Heavyweight Baby Galaxies

Astronomers looking at galaxies in the universe’s distant past were surprised to find some compact, very young galaxies that have masses similar to a mature, grown-up galaxy. Using the Hubble Space Telescope, astronomers discovered nine small galaxies, each weighing in at 200 billion times the mass of the Sun. The galaxies, each only 5,000 light-years across, are a fraction of the size of today’s adult galaxies but contain approximately the same number of stars. Each galaxy could fit inside the central hub of our Milky Way Galaxy.

Using the Hubble in conjunction with Keck Observatory in Hawaii, astronomers were able to study the galaxies as they existed 11 billion years ago, when the Universe was less than 3 billion years old.

“Seeing the compact sizes of these galaxies is a puzzle”, said Pieter G. van Dokkum of Yale University in New Haven, Connecticut, USA, who led the study. “No massive galaxy at this distance has ever been observed to be so compact. These galaxies would have to change a lot over 11 billion years, growing five times bigger. They could get larger by colliding with other galaxies, but such collisions may not be the complete answer. It is not yet clear how they would build themselves up to become the large galaxies we see today.”

To determine the sizes of the galaxies, the team used the Near Infrared Camera and Multi-Object Spectrometer on Hubble. For the Keck observations, a powerful laser was used to correct for image blurring caused by the Earth’s atmosphere. Only Hubble, Keck and ESO’s Very Large Telescope are really able to measure the sizes of these galaxies as they are very small and far away.

The ultra-dense galaxies might comprise half of all galaxies of that mass 11 billion years ago, van Dokkum said, forming the building blocks of today’s largest galaxies.

How did these small, crowded galaxies form? One way, suggested van Dokkum, involves the interaction of dark matter and hydrogen gas in the nascent Universe. Dark matter is an invisible form of matter that accounts for most of the Universe’s mass. Shortly after the Big Bang, the Universe contained an uneven landscape of dark matter. Hydrogen gas became trapped in pockets of the invisible material and began spinning rapidly in dark matter’s gravitational whirlpool, forming stars at a furious rate.

Based on the galaxies’ mass, which is derived from their color, the astronomers estimated that the stars are spinning around their galactic disks at roughly 400 to 500 kilometers per second. Stars in today’s galaxies, by contrast, are traveling at about half that speed because they are larger and rotate more slowly than the compact galaxies.

The astronomers say that these galaxies are ideal targets for the Wide Field Camera 3, which is scheduled to be installed aboard Hubble during upcoming Servicing Mission 4 in the fall of 2008.

Original News Source: European Hubble Space Telescope Homepage

New Hubble Images Reveal Plethora of Interacting Galaxies

59 new images from the Hubble Space Telescope show some very unusual but incredibly spectacular colliding galaxies. Colliding or interacting galaxies are found throughout the Universe, and sometimes these collisions trigger bursts of star formation, or the mergers form new galaxies. The image above shows the aftermath of an encounter between two galaxies, resulting in a ring-shaped galaxy and a long-tailed companion. Officially called Arp 148, it also has the nickname ‘Mayall’s object.’ It is located in the constellation of Ursa Major, the Great Bear, approximately 500 million light-years away. These images are the largest collection from Hubble ever published simultaneously, and they celebrate the 18th anniversary of Hubble’s launch. And there’s more….


This is a stunning snapshot of a celestial dance performed by a pair of similar sized galaxies. ESO 77-14 is in the constellation of Indus, the Indian, some 550 million light-years away from Earth. The galaxy on the right has a long, bluish arm while its companion has a shorter, redder arm.

The Hubble Site has a video about colliding galaxies.

For the entire collection of these images see the Hubble site.

Original News Source: ESA press release

Hubble Finds Dozens of Gravitationally Lensed Galaxies

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One of the breakthroughs in modern astronomy is the use of gravitational lenses, where a closer galaxy or star focuses the light from a more distant object. The more astronomers look, the more they find these helpful objects, allowing them to peer at objects much further away. The number of known gravitationally-lensed galaxies jumped up today, when astronomers announced another 67 new lenses.

These 67 lenses were part of the COSMOS project; a detailed survey of small region of the sky about the same as 9 times the area of the Moon. Both Earth and space-based telescopes are working together to provide a survey of the sky which is very deep. And one of the key instruments in the project is the Hubble Space Telescope.

One of the big surprises of this survey is just how many lenses turned up in such a small area of the sky. Based on this discovery rate, researchers think that there could be 500,000 similar gravitationally-lenses galaxies out there.

At least 4 of the lenses are Einstein rings. This is a situation where the foreground and background galaxy are lined up so perfectly, the distorted distant galaxy forms a ring around the closer one.

In order to find the lenses, astronomers had to sift through a collection of 2 million candidate galaxies. Then the researchers had to look through each COSMOS image by eye and identify any potentially strong gravitational lenses. Finally, they checked both the foreground and background galaxy to make sure that they’re really two separate objects separated by billions of light years, and not just a strangely shaped galaxy.

Now that the researchers have so many gravitational lenses, they can do some really interesting things. For example, they’ll be able to study the dark matter distribution around the galactic lenses. And they’ll also be able to start accumulating a census of galaxy masses to see if they match predictions.

Original Source: Hubble News Release

Hubble Finds One of the Earliest, Brightest Galaxies in the Universe

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By boosting the abilities of Hubble with a gravitational lens telescope provided by nature, astronomers have been able to peer back to the earliest times in the Universe; to see a galaxy just 700 million years after the Big Bang.

The newly forming galaxy (well, it was newly forming 13 billion years ago) is called A1689-zD1, and appears to be undergoing furious levels of star formation. Just a few hundred million years before this, the Universe was in the dark ages, when the Universe’s hydrogen cooled and formed thick clouds of hydrogen. This hydrogen acted like a fog, obscuring everywhere.

Although it’s tremendously powerful, the Hubble Space Telescope wasn’t strong enough to image the galaxy. It took the additional gravity of the nearby Abel 1689 cluster to act as a natural lens and magnify the light coming from A1689-zD1. With this technique, astronomers were able to increase its brightness by a factor of 10.

The hope is that this galaxy will give astronomers valuable insights into the formative years of galaxy birth and evolution. One of these questions is: what ended the dark ages?

“This galaxy presumably is one of the many galaxies that helped end the dark ages,” said astronomer Larry Bradley of Johns Hopkins University in Baltimore, Md., and leader of the study. “Astronomers are fairly certain that high-energy objects such as quasars did not provide enough energy to end the dark ages of the universe. But many young star- forming galaxies may have produced enough energy to end it.”

The studies show that this galaxy is probably a good example of what most galaxies looked like in the early Universe. It’s just a fraction of the mass of the Milky Way, but it has high rates of star formation. Much of this star formation is happening in very tiny regions compared to the size of the final galaxy.

Obviously, with Hubble straining at its limits to see this galaxy at all, it can’t make out individual stars, only knots of the brightest ones. But future telescopes, such as the James Webb Space Telescope, is ideally suited to take a much deeper look at it. It would also make a good target for the Atacama Large Millimeter Array, which will become the most powerful radio telescope in the world when it’s completed in 2012.

Original Source: Hubble News Release

Hubble Sees an Ancient Elliptical Galaxy

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As galaxies come together through successive mergers they take on the splendid spiral shape like our own Milky Way. Keep merging those larger galaxies, though, and you’ll eventually get an elliptical galaxy – a gigantic diffuse cloud of ancient stars with little structure. Such a galaxy, NGC 1132, was recently photographed by the Hubble Space Telescope.

The elliptical galaxy NGC 1132 belongs in this class of galaxies called “giant ellipticals”. And the galaxy, with its constellation of dwarf galaxies is known as a “fossil group”. They’re the remnants and wreckage from past collisions between large galaxies.

In visible light, NGC 1132 looks like a single, isolated galaxy. But using a technique called gravitational lensing to map out the surrounding dark matter, astronomers found that it resides in a huge cloud of the stuff. In fact, NGC 1132 has as much dark matter as you might find in a group of tens or even hundreds of galaxies.

And once again, in visible light, its stars extend 120,000 light years from its centre. But in the X-ray spectrum, the glow extends 10 times as far – again, similar to a group of galaxies.

So where do fossil groups like this come from? Astronomers think they’re the end product of cosmic collisions, where a single large galaxy consumes all of its neighbors. It’s also possible they’re the result of a strange process, where something stopped moderate galaxies from forming, and only a single large galaxy came together in that region of space.

By analyzing galaxies like this, astronomers will get a better sense of galaxy evolution. It’ll help predict what’s going to happen when the Milky Way and Andromeda collide billions of years in the future.

Original Source: ESA/Hubble News Release

Supercluster Ruled By the Pull of Dark Matter

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Enough of this small stuff, let’s look at the big picture. The really really big picture. In this case, one of the largest patches of the sky ever observed by the Hubble Space Telescope. A new detailed survey was released today that combines 80 separate Hubble images together. In addition to a framework of galaxy clusters, the images show the distribution of dark matter that holds the clusters together – and tears it all apart.

The dark matter survey is part of the Space Telescope Abell 901/902 Galaxy Evolution Survey (STAGES), which looks at one of the larger structures in the Universe: the Abell 901/902 superclusters. This is a region of tremendous violence and chaos. Galaxies are being pulled into the core of the superclusters, and getting distorted and stripped of their gas and dust.

And one of the primary forces of this violence comes from the completely invisible dark matter that makes up the bulk of the matter in the region. Instead of being equally distributed, though, this dark matter has pooled into enormous clumps.

An international team of astronomers used Hubble to measure how individual galaxies are distorted by clouds of dark matter. The dark matter is invisible, but it does have mass, which can pull at the light as it moves past. The astronomers know what different galaxies should probably look like, and then can figure out how much dark matter is in between, distorting the view. It’s actually pretty incredible to see the dark matter map imposed over top of the visible light image.

“Thanks to Hubble’s Advanced Camera for Surveys, we are detcting for the first time the irregular clumps of dark matter in this supercluster,” said Catherine Heymans of the University of British Columbia. “We can even see an extension of the dark matter toward a very hot group of galaxies that are emitting X-rays as they fall into the densest cluster core.”

The Hubble study identified 4 separate regions where the dark matter has pooled into dense clumps, adding up to 100 trillion times the mass of the Sun. They can even make out irregular clumps of dark matter in the supercluster. These areas match the locations where hundreds of old galaxies have already experienced the violent passage from the outskirts of the supercluster into the denser regions.

Original Source: Hubble News Release

The Plan to Fix Hubble

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Although the space shuttles have a busy schedule completing the construction of the International Space Station, there’s one other job to complete – servicing the Hubble Space Telescope. NASA officials announced the details of the mission today at the Winter meeting of the American Astronomical Society. If all goes well, the space shuttle Atlantis will visit Hubble some time around August 2008, carrying 7 astronauts and the spare parts they need to bring Hubble back to top-notch condition.

Over the course of 11 days, the astronauts will perform a total of 5 spacewalks. During these trips to service Hubble, the astronauts will install two new science instruments, upgrade existing instruments and replace failing gyroscopes, batteries and thermal blankets. Atlantis will also reboost the telescope’s decaying orbit.

One of the most critical jobs will be to repair the telescope’s Advanced Camera for Surveys (ACS). This is the visible light instrument that produces the pretty pictures that have made Hubble so famous. The instrument suffered a power failure in January 2007.

With this collection of upgrades, Hubble’s life should be extended to 2013. David Leckrone, Senior Hubble Project Scientist noted that “when the astronauts leave Hubble for the last time, it will be at the apex of its capabilities – better than it has ever been before.” In fact, with these upgrades, Hubble should be 90X more sensitive than before.

One of the unique challenges of this mission will be for the astronauts to repair components that were never designed for orbital repair. In some cases, the astronauts will need to open up boxes and replace circuit boards.

Lead astronaut John Grunsfeld explained just how complex the task of repairing the Advanced Camera for Surveys is going to be, “we’re going to do something that’s never been done before. We’re going to swap circuit boards. We’re going to be working with hundreds of number 4 torque screws. These are really tiny screws. Whatever you do, don’t lose a screw inside the telescope. I have to cut an electromagnetic blanket on the Advanced Cameras for Surveys which could leave sharp edges. We’re astronauts, wearing balloons of air around us, and we don’t like sharp edges. With that removed, I then have to remove 36 of these screws. But they’re at an angle, so I won’t be able to see or reach them easily. I’ve been training in an underwater tank, and plan to get to know each of these screws.”

To demonstrate the tools he’s going to be working with, John Grunsfeld wore his astronaut gloves during his presentation in today’s press conference. “I figured I needed as much practice with these gloves as possible.”

Even the death of Hubble is being arranged. At some point in 2020, when the telescope finally reaches the end of its enhanced lifetime, NASA intends to dock a rocket to the telescope and then drive it into the ocean. As part of this process, the astronauts will install a special docking module, so the deorbiting rocket can attach easily and complete its grim task.

Hubble’s View of M74

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During many holidays, the folks working on NASA’s Hubble Space Telescope try and find an image that captures the essence of the celebration. We’ve seen Christmas Tree clusters and spooky nebulae. To show their holiday spirit, the Hubble folks have released this beautiful image of the spiral galaxy M74. It’s a stretch, I guess, but wow, what a picture.

From the original Hubble news release, here’s how they describe the photograph.

Hubble has sent back an early Christmas card with this new NASA/ESA Hubble Space Telescope image of the nearby spiral galaxy Messier 74. It is an enchanting reminder of the impending season. Resembling glittering baubles on a holiday wreath, bright knots of glowing gas light up the spiral arms; regions of new star birth shining in pink.

Messier 74 is one of the best examples we can see of a “grand design” spiral galaxy, much like our own Milky Way. In the case of M74, it’s conveniently facing face on, so we can see intricate details in all parts of the galaxy’s structure.

The bright pink areas in the spiral arms are huge, short lived clouds of hydrogen gas glowing from the newborn stars inside them. The dark dust lanes that extend out along the spiral arms contain a new generation of blue stars.

M74 was first discovered by the French astronomer Pierre Mechain in 1780, and then added to Charles Messier’s famous catalogue of deep sky objects. Of all the objects in the catalogue, it’s one of the faintest, and has been nicknamed “The Phantom Galaxy” by amateur astronomers trying to spot it in their telescopes.

So thanks Hubble, feel free to celebrate any holiday, celebration or random even you like. Just keep the pictures coming.

Original Source: Hubble News Release