Galactic Ghosts Haunt Their Killers

Image of the stellar tidal stream surrounding the spiral galaxy NGC 5907 obtained with an amateur robotic telescope in the mountains of New Mexico. (R. Jay Gabany)

The title may sound dramatic, but it is very descriptive. New observations of two galaxies have shown huge streams of stars, not belonging inside those galaxies, reaching out into space. These streams are all that are left of galaxies that are now dead, eaten by their cannibal neighbour, now sitting in their place. The streams form an eerie halo around their killers, looking like ghosts of their former selves…

So what happened to these ill-fated galaxies? Galactic cannibalism is what happened. In both examples, large spiral galaxies have overrun smaller dwarf galaxies, devouring most of their stars. All that is left are the huge fossilized remains in the form of a tenuous distribution of dim, old, metal-poor stars. Judging by the lack of galactic structure in these “ghosts”, the cannibalizing spiral galaxies have been very efficient at eating their smaller dwarf cousins.

a gigantic, tenuous loop-like structure extending more than 80 000 light-years from the centre of the galaxy (towards the top left). (R. Jay Gabany)

The debris surrounding NGC 5907 (approximately 40 million light-years from Earth) extends 150,000 light-years across (pictured top). NGC 5907 destroyed one of its dwarf satellite galaxies at least 4,000 million years ago, consuming the stars, star clusters and dark matter, leaving only a small number of old stars behind to form a complicated criss-cross pattern of galactic fossils.

Our results provide a fresh insight into this spectacular phenomenon surrounding spiral galaxies and show that haloes contain fossil dwarf galaxies, thus providing us with a unique opportunity to study the final stages in the assembly of galaxies like ours.” – David Martínez, from the Instituto de Astrofísica de Canarias (IAC) leading the team that carried out these observations.

In the second spiral galaxy, NGC 4013 (50 million light-years from Earth in the constellation of Ursa Major), the ghost of another dead dwarf galaxy stretches 80,000 light-years across and is made up of old stars. Its 3D geometry is unknown, but it has similar characteristics to the Monoceros tidal stream which surrounds the Milky Way. The Monoceros tidal stream is a ring of stars, originating from a local dwarf galaxy that was eaten by our galaxy over 3,000 million years ago.

These images have a huge amount of science to offer researchers. Primarily, the detection of these galactic fossils confirms the predictions of the cold dark matter model of cosmology, which describes how the large spiral galaxies were formed from merging stellar systems.

“…fitting theoretical models to these star streams enables us to reconstruct their history and describe one of the most mysterious and controversial components of galaxies: dark matter.” – Jorge Peñarrubia, theoretical astrophysicist at the University of Victoria (Canada) who is working on this project.

Source: IAC

The Pioneer Anomaly: A Deviation from Einstein Gravity?

Artist impression of the Pioneer 10 probe (NASA)

Both Pioneer probes are approximately 240,000 miles (386,000 km) closer to the Sun than predicted by calculation. Scientists have been arguing over the cause of this mysterious force for a decade and reasons for the Pioneer anomaly range from the bizarre to the sublime. Is it a simple fuel leak, pushing the probes of course? Is it phantom dark matter dragging them down? Or do the gravity textbooks need to be re-written? Unfortunately there’s still no one answer, but some researchers believe there might be a small deviation in the large-scale space-time Einstein described in his famous theory of general relativity. See, I knew there would be a simple explanation…

The Pioneer 10 and 11 deep space probes were launched in 1972 and 1973, visiting Jupiter and Saturn before pushing on toward interplanetary space, into the unknown. The Pioneer program really lived up to its name, pioneering deep space exploration. But a few years on, as the probes passed the through the 20-70 AU mark, something strange happened… not suddenly, but gradually. Ten years ago Pioneer scientists noticed that something was wrong; the probes were slightly off course. Not by much, but both were experiencing a slight but constant sunward acceleration. The Pioneer probes had been measured some 240,000 miles (386,000 km) closer to the Sun than predicted. This might sound like a long way, but in astronomical terms it’s miniscule. 240,000 miles is a tiny deviation after 6.5 billion miles (10.5 billion km) of travel (it would take light 10 hours to cover this distance), but it’s a deviation all the same and physicists are having a very hard time trying to work out what the problem is.

That is until NASA physicist Slava Turyshev, co-discoverer of the anomaly, rescued a number of Pioneer magnetic data storage disks from being thrown out in 2006. These disks contain telemetric data, temperature and power readings that both Pioneer probes had transmitted back to mission control up to 2003 (when Pioneer 10 lost contact with Earth). From this, Turyshev and his colleagues teamed up with Viktor Toth, a computer programmer in Ottawa, Ontario, to design a new code designed to extract the vast quantity of raw binary code (1s and 0s), revealing the temperature and power readings from the crafts instruments. It sounds as if the search for the culprit of the Pioneer anomaly required a bit of forensic science.

Now the researchers have a valuable tool at their disposal. Turyshev and 50 other scientists are trying to match this raw data with modelled data in an effort to reconstruct the heat and electricity flow around the craft’s instrumentation. Electricity was supplied by the on-board plutonium generator, but this is only a small portion of the energy generated; the rest was converted to heat, lost to space and warmed up the probe’s bodywork. Heat lost to space and warming of the probe’s instruments are both thought to have a part to play in altering spacecraft momentum. So could this be the answer?

Tests are ongoing, and only a select few simulations have been run. However, early results indicate that around 30% of the Pioneer anomaly is down to the on-board heat distribution. The rest, it seems, still cannot be explained by probe dynamics alone. The team are currently processing a total of 50 years of telemetry data (from both Pioneer 10 and 11), so more simulations on the rich supply of transmissions from the probes may still uncover some surprises.

But on the back of everyone’s mind, and it keeps cropping up in every Pioneer anomaly article I find, that the fundamental physics of our universe may need to be brought into question. Sending long-distance deep space probes gives us a huge opportunity to see if what we observe locally is the same for other parts of the Solar System. Could Einstein’s general theory of relativity need to be “tweaked” when considering interplanetary (or interstellar) travel?

The researchers are excited if a mundane solution does not present itself (i.e. probe heat distribution effects), therefore indicating some other cosmic reason is behind this anomaly:

If we actually had a means in the solar system here to measure deviations from Einstein’s gravity, that would be phenomenal.” – Viktor Toth

In the mean time, Pioneer 10 is drifting silently toward the red star of Aldebarran and (barring any more anomalous behaviour) will arrive there in 2 million years time…

Sources: Scientific American, Symmetry Breaking News

Radiation Sickness, Cellular Damage and Increased Cancer Risk for Long-term Missions to Mars

A mission to Mars will benefit from a mini-magnetosphere (NASA)

There is a nagging problem under the surface of the excitement surrounding the future of long-term missions into space. Human exposure to the high amounts of solar radiation and other sources of cosmic rays is likely to be the main factor that could curtail mankind’s dreams for future manned settlements on other planets. The effects of radiation exposure to astronauts is not fully understood, but could range from acute radiation sickness (perhaps after being caught in an intense solar storm during interplanetary transit) to gradual cellular damage, greatly increasing the risk of cancer in long-term missions. So what can we do about it? Mankind is highly adaptive and some countermeasures are gradually being realized. (And yes, the Russian Space Monkeys might be able to help…)

The problem comes when humans leave the protective blanket of the Earth’s magnetic field. Acting like a huge, invisible force field, the magnetosphere deflects most of the harmful high energy particles being fired from the Sun. Anything that penetrates this barrier is quickly absorbed by our thick atmosphere. Even at high altitudes, in low Earth orbit, some protection to astronauts can be provided (although the ambient radiation is far higher up there than down here). So when we talk about colonizing other planets and sending astronauts further and further into deep space, radiation exposure becomes a bigger risk.

Solar flares will be a problem for future colonists (SOHO/EIT)

An immediate concern is that astronauts may get caught in a solar storm, where the Sun (usually around solar maximum) ejects huge clouds of highly energetic protons. If the storm is intense enough, huge doses of radiation could be inflicted on the men and women in space. Roughly, a dose of 500 rads or more will kill a human in two to three hours, and a smaller dose could cause acute radiation sickness. Radiation sickness could be fatal in weeks should the astronaut not receive urgent medical care. How about the long-term, gradual impact of prolonged exposure to higher-than-normal doses of radiation? This is an area of space medicine that we do not completely understand as yet.

In new research by the Lombardi Comprehensive Cancer Center at Georgetown University Medical Center, the high-energy nature of radiation in space may lead to premature aging and prolonged oxidative stress in cells. This also suggests that astronauts risk a higher than normal risk of cancers, such as colon cancer, through exposure to “high linear energy transfer” (LET) radiation. LET radiation consists of the high energy protons emitted by the Sun and cause a huge amount of damage to small areas of tissue.

Radiation exposure, either intentional or accidental, is inevitable during our lifetimes, but with plans for a mission to Mars, we need to understand more about the nature of radiation in space. There is currently no conclusive information for estimating the risk that astronauts may experience.” – Kamal Datta, M.D., assistant professor at Lombardi and lead author.

With NASA’s Project Constellation on the horizon, there has been a focus on the long-term effects of interplanetary radiation. Ultimately, this project aims to send humans to the Moon and Mars, but there are strong indicators that astronauts will face in increased cancer risk and lifespan reduction, a massive hindrance to a mission spanning several months or a thriving proto-settlement.

This is where the lab mice help us out. The amount of “free radicals” (highly reactive molecules often linked with cancer and cell aging) were measured and found that the mice developed highly oxidative (i.e. full of free radical molecules) gastrointestinal tracts when exposed to space-like high-LET radiation. The Lombardi group concluded that the mice had developed a high risk to various cancers, particularly gastrointestinal cancers. They also noticed that after exposure (even after two months), the mice prematurely aged, signifying that the effect of radiation damage can persist long after exposure to a high-LET environment.

So what can we do? There are several plans in motion to further test the effects of radiation on humans and to predict when astronauts will be at risk. This week, Russia announced (controversial) plans to send monkeys back into space, possibly as far as Mars. Once the shock of this “outdated” proposal wore off (the previous Russian space monkey program ran out of funding in the 1990’s), it became very clear as to what the Russian space agency is hoping to achieve: to have a better understanding of the long-term exposure to a high-LET environment on the human physiology. Many will argue that this practice is cruel and unnecessary, but others will say monkeys are used in experiments every day, why shouldn’t they help us in the ultra-modern world of space travel? The jury is still out on this debate, but there are many ways to investigate and counteract the radiation effect on humans.

Energetic particle tracks in a bubble chamber (NASA)

There are also many systems in place to protect mankind from the onslaught of solar storms. Using the Solar and Heliospheric Observatory (SOHO) and other craft located between the Earth and Sun, an early warning system has been set up to provide astronauts on orbit with some time to take cover should a solar flare be launched Earth-bound. This system is fully operational and has already proven itself. Recently, I toyed with the idea of a similar Mars-based early warning system, providing future Mars colonies with about 40 minutes advanced notice of an incoming solar storm.

Shielding is another obvious protective measure. Lunar and Mars colonies are most likely going to use large amounts of regolith to block the incoming particles. Only a few meters of locally dug-up regolith will provide excellent protection. But what about the journey to Mars? How will the astronauts of projects such as Constellation be protected? Perhaps an advanced “Ion Shield” might work?

Whatever the effect of radiation on humans in space, it seems obvious that we are in the infancy of space flight and we are already addressing some of the most difficult problems. Over the next few years, much effort will be focused on the health of astronauts, hopefully finding some answers to the space radiation problem.

Original source: Georgetown University Medical Center

Latest News on Apophis: 13 -year-old Boy Corrects NASA’s Estimates of Earth Impact — Not! (Update)

Annimation of Apophis.  Image Credit:  Osservatorio Astronomico Sormano
Update: It turns out this story is a fabrication and AFP didn’t check the facts with NASA as I suspected. According to the blog Cosmos4u, they talked with Don Yeomans at NASA’s NEO office and this is what Yeoman’s said about the news story of a 13-year old boy correcting NASA’s estimates of Apohpis impacting earth: “We have not corresponded with this young man and this story is absurd, a hoax or both. During its 2029 Earth close approach, Apophis will approach the Earth to about 38,900 km, well inside the geosynchronous distance at 42,240 km. However, the asteroid will cross the equatorial belt at a distance of 51,000 km – well outside the geosynchronous distance. Since the uncertainty on Apophis’ position during the Earth close approach is about 1500 km, Apophis cannot approach an Earth satellite. Apophis will not cross the moon’s orbital plane at the Moon’s orbital distance so it cannot approach the moon either.”

Also, the scientist mentioned in AFP’s story said he wasn’t conferred with either by the news agency. So don’t give any heed to this story that has been running amok around the internet.

But here’s our story on this as it originally ran: Here’s a story that supports the value of science fairs. And it also makes one wonder where else NASA’s decimal points might be off by a couple of places. One caveat on this news piece, however: as far as I know there hasn’t been an official NASA press release on this.

Reportedly, a 13-year-old German schoolboy doing research for a science competition found errors in NASA’s estimates on the chances of the asteroid Apophis colliding with Earth. The boy, Nico Marquardt used data from the Institute of Astrophysics in Potsdam to calculate that there was a 1 in 450 chance that the Apophis asteroid will collide with Earth. NASA had previously estimated the chances at only 1 in 45,000, but according to an AFP news release, NASA now acknowledges the kid is right. (Actually, no they don’t.)
Continue reading “Latest News on Apophis: 13 -year-old Boy Corrects NASA’s Estimates of Earth Impact — Not! (Update)”

Where In The World (and What World) Is This?

Anyone care to guess what orbiting spacecraft is responsible for taking this image, or even what world this is a picture of? At first glance, with all those craters, it could be Mars. However, the coloring isn’t quite right for the Red Planet. Is it a photograph of Mercury or an image of the moon?

OK, yes, this is an image of Earth, but you were wondering there for awhile, weren’t you! Interestingly enough, the white area is not snow, and the craters are not impact craters, but volcanic. And what spacecraft gets credit for the image? The International Space Station. This is one of the most recent images taken by the astronauts on board the ISS as part of the Earth Observatory program. A wonderful website, NASA’s Gateway to Astronaut Photography of Earth, hosts an incredible collection of photographs that astronauts have taken of our home planet.

Beginning with the Mercury missions in the early 1960s, astronauts have taken photographs of the Earth. As of April 7, 2008, this website has 759,527 views of the Earth, which includes 315,923 from the ISS. The site processes images coming down from the International Space Station on a daily basis, so the database is continually growing. The U.S. Destiny Laboratory module has a science window with high optical quality, which usually faces the Earth, and most of the ISS’s images are taken from that window on the world. On board the ISS is a nice selection of professional digital cameras, and a variety of lenses. One could spend hours (or days or a lifetime!) browsing through the striking photographs of Earth the astronauts have taken. The website also includes lots of information about each of the images, and a fun Where In the World quiz to test your geographical knowledge.

The image above is of the Harrat Khaybar volcanic field, a 14,000-square-kilometer area located in the western Arabian peninsula. The volcanic field was formed by eruptions along a 100-kilometer, north-south vent system over the past 5 million years. The most recent recorded eruption took place between 600-700 AD.

Harrat Khaybar contains a wide range of volcanic rock types and spectacular landforms, several of which are represented in this astronaut photograph. There are dark, fluid basalt lava flows, and the white deposits are sand and silt that accumulate in the depressions. There are lava domes and cones from the past volcanic activity.

The ISS astronauts take images daily of our planet. The image of Harrat Khaybar was taken on March 31, 2008, with a Kodak 760C digital camera fitted with a 400 mm lens, and is provided as part of the the ISS Crew Earth Observations experiment.

Original News Source: Earth Observatory website

Astrosphere for April 15, 2008

Don’t just look inward, look outward. There’s a whole astrosphere out there. Your picture for the day is Saturn (of course), captured by Stargazer 7000.

Astronomy Picture of the Day has a beautiful shot of the night sky over Sweden.

PZ Myers has spoken and I must obey. Here’s all you need to know about expelled.

And here’s a review for another movie, Dark Matter.

Speaking of dark matter, Ethan Siegel explains the practical uses for his research.

Astroprof recalls famed astronomer John Archibald Wheeler; the man who coined the term “black hole” passed away this week.

Bad Astronomer Phil Plait celebrated Yuri’s night, in style.

Coolest, Darkest Brown Dwarf Discovered

An artist impression of a brown dwarf (Hallinan et al., NRAO/AUI/NSF)

The coolest brown dwarf has been discovered, with a surface temperature of 623 Kelvin (that’s only 350 Celsius or 660 degrees Fahrenheit). Compare with the surface temperature of our Sun, a modest 6,000 Kelvin, you can see that this featherweight dwarf “star” is a little odd. As far as stars go, this one is pretty unspectacular, but it does hold a vast amount of interest. It may not be as sexy as a supernova or as exotic as a neutron star, the humble brown dwarf may provide the essential link between planets (specifically gas giants) and stars. They are effectively failed stars, and this new discovery demonstrates just how cold they can be…

Brown dwarfs are the link between massive planets and small stars. They have an upper limit of about 80 Jupiter masses, but are not massive enough to sustain nuclear fusion in their core. They do however experience convection from the interior to the surface. The confusion arises when trying to find the lower limit of brown dwarf size, at what mass does the gas giant planet start being a brown dwarf star? This grey area is thought to be characterized by an entirely new stellar type: Y-class dwarfs. Until now Y-class dwarfs have been very elusive and have only existed in theory.

A comparison of the size of Jupiter, a brown dwarf, a small star and the Sun (Gemini Observatory/Artwork by Jon Lomberg)

Astronomers using near-infrared and infrared instruments at the Canada France Hawaii and Gemini North telescopes and the European Southern Observatory in Chile have discovered a Y-class dwarf, bringing this strange failed star from theory and into reality. What’s more, it’s in our cosmic neighbourhood, only 40 light-years from Earth. This brown dwarf has been unglamorously named “CFBDS0059”, but I would have called it something like “The Dark Star” or “The Death Star”, as it is so dim and its surface temperature is approximately the same as the surface temperature of the planet Mercury (but much cooler than the surface temperature of Venus). As it is so cool, it isn’t very luminescent and only radiates in the near-infrared wavelengths (it’s not even as hot as a standard electric stove element), requiring specialist equipment to detect it. As it turns out, CFBDS0059 is small, only 15-30 times the mass of Jupiter, fulfilling the lower mass limit of brown dwarf stars and will be known as the first Y-class dwarf to be observed.

But what is the indicator that a Y-class brown dwarf has been observed? Using spectrometers, astronomers have been able to see the constituent compounds making up the brown dwarf’s atmosphere. Should ammonia be discovered, it’s a pretty sure sign that a Y-class dwarf has been found.

We are starting to see a little hint of ammonia absorption.” Loic Albert (stellar researcher) of the Canada France Hawaii Telescope in Hawaii, commenting on CFBDS0059.

There are two other verified classes of dwarfs, L and T-class dwarfs. L-class dwarfs are hotter, with temperatures from 2200 to 3600°F and T-class dwarfs are cooler than 2190°F and methane-rich. CFBDS0059 is obviously much, much cooler, but researchers believe there may be still cooler dwarfs out there, possibly condensing any water vapour in their atmospheres to form clouds, setting Y-class dwarfs far from the characteristics of its L and T-class cousins. Should they get any colder, water will freeze into ice crystals, giving them more planetary than stellar characteristics.

Source: Discovery.com

Milky Way’s Black Hole Gave Off a Burst 300 Years Ago

Sagittarius A*. Image credit: Chandra

Our Milky Way’s black hole is quiet – too quiet – some astronomers might say. But according to a team of Japanese astronomers, the supermassive black hole at the heart of our galaxy might be just as active as those in other galaxies, it’s just taking a little break. Their evidence? The echoes from a massive outburst that occurred 300 years ago.

The astronomers found evidence of the outburst using ESA’s XMM-Newton space telescope, as well as NASA and Japanese X-ray satellites. And it helps solve the mystery about why the Milky Way’s black hole is so quiet. Even though it contains 4 million times the mass of our Sun, it emits a fraction of the radiation coming from other galactic black holes.

“We have wondered why the Milky Way’s black hole appears to be a slumbering giant,” says team leader Tatsuya Inui of Kyoto University in Japan. “But now we realize that the black hole was far more active in the past. Perhaps it’s just resting after a major outburst.”

The team gathered their observations from 1994 to 2005. They watched how clouds of gas near the central black hole brightened and dimmed in X-ray light as pulses of radiation swept past. These are echoes, visible long after the black hole has gone quiet again.

One large gas cloud is known as Sagittarius B2, and it’s located 300 light-years away from the central black hole. In other words, radiation reflecting off of Sagittarius B2 must have come from the black hole 300 years previously.

By watching the region for more than 10 years, the astronomers were able to watch an event wash across the cloud. Approximately 300 years ago, the black hole unleashed a flare that made it a million times brighter than it is today.

It’s hard to explain how the black hole could vary in its radiation output so greatly. It’s possible that a supernova in the region plowed gas and dust into the vicinity of the black hole. This led to a temporary feeding frenzy that awoke the black hole and produced the great flare.

Original Source: ESA News Release

Binoculars for Astronomy

Astronomy is best when you get outside and look into the skies with your own eyes. And the best way to get started is with a set of binoculars for astronomy. They’re light, durable, easy to use, and allow you to see objects in the night sky that you just couldn’t see with your own eyes. There are so many kinds of binoculars out there, so we’ve put together this comprehensive guide to help you out.

Everyone should own a pair of binoculars. Whether you’re interested in practicing serious binocular astronomy or just want a casual cosmic close-up, these portable “twin telescopes” are both convenient and affordable. Learning more about how binoculars work and what type of binoculars work best for astronomy applications will make you much happier with your selection. The best thing to do is start by learning some binocular “basics”.

What are binoculars and how do they work?
Binoculars are both technical and simple at the same time. They consist of an objective lens (the large lens at the far end of the binocular), the ocular lens (the eyepiece) and a prism (a light reflecting, triangular sectioned block of glass with polished edges).

The prism folds the light path and allows the body to be far shorter than a telescope. It also flips the image around so it doesn’t look upside-down. The traditional Z-shaped porro prism design is well suited to astronomy and consists of two joined right-angled prisms which reflects the light path 3 times. The sleeker, straight barrelled roof prism models are more compact and far more technical. The light path is longer, folding 4 times and requires stringent manufacturing quality to equal the performance. These models are better suited to terrestrial subjects, and are strongly not recommended for astronomy use.

If you’re using binoculars for astronomy, go with a porro prism design.

Choosing the Lens Size
Every pair of binoculars will have a pair of numbers associated with it: the magnifying power times (X) the objective lens size. For example, a popular ratio is 7X35. For astronomical applications, these two numbers play an important role in determining the exit pupil – the amount of light the human eye can accept (5-7mm depending on age from older to younger). By dividing the objective lens (or aperture) size by the magnifying power you can determine a pair of binoculars exit pupil.

Like a telescope, the larger the aperture, the more light gathering power – increasing proportionately in bulk and weight. Stereoscopic views of the night sky through big binoculars is an incredible, dimensional experience and one quite worthy of a mount and tripod! As you journey through the binocular department, go armed with the knowledge of how to choose your binoculars lens size.

Why does the binocular lens size matter? Because binoculars truly are a twin set of refracting telescopes, the size of the objective (or primary) lens is referred to as the aperture. Just as with a telescope, the aperture is the light gathering source and this plays a key role in the applications binoculars are suited for. Theoretically, more aperture means brighter and better resolved images – yet the size and bulk increases proportionately. To be happiest with your choice, you must ask yourself what you’ll be viewing most often with your new binoculars. Let’s take a look at some general uses for astronomy binoculars by their aperture.

Different Sizes of Binoculars
Binoculars with a lens size of less that 30mm, such as 5X25 or 5X30, are small and very portable. The compact models can fit easily into a pocket or backpack and are very convenient for a quick look at well-lit situations. In this size range, low magnifications are necessary to keep the image bright.

Compact models are also great binoculars for very small children. If you’re interested in choosing binoculars for a child, any of these models are very acceptable – just keep in mind a few considerations. Children are naturally curious, so limiting them to only small binoculars may take away some of the joy of learning. After all, imagine the thrill of watching a raccoon in its natural habitat at sundown… Or following a comet! Choose binoculars for a child by the size they can handle, whether the model will fold correctly to fit their interpupilary size, and durability. Older children are quite capable of using adult-sized models and are naturals with tripod and monopod arrangements. For less than the price of most toys, you can put a set of quality optics into their hands and open the door to learning. Children as young as 3 or 4 years old can handle 5X30 models easily and enjoy wildlife and stargazing both!

Binocular aperture of up to 40mm is a great mid-range size that can be used by almost everyone for multiple applications. In this range, higher magnification becomes a little more practical. For those who enjoy stargazing, this is an entry level aperture that is very acceptable to study the Moon and brighter deep sky objects and they make wonderful binoculars for older children.

Binoculars up to 50-60mm in lens size are also considered mid-range, but far heavier. Again, increasing the objective lens size means brighter images in low light situations – but these models are a bit more bulky. They are very well suited to astronomy, but the larger models may require a support (tripod, monopod, car window mount) for extended viewing. Capable of much higher magnification, these larger binocular models will seriously help to pick up distant, dimmer subjects such as views of distant nebulae, galaxies and star clusters. The 50mm size is fantastic for older children who are ready for more expensive optics, but there are drawbacks.

The 50-60mm binoculars are pushing the maximum amount of weight that can be held comfortably by the user without assistance, but don’t rule them out. Available in a wide range of magnifications, these models are for serious study and will give crisp, bright images. Delicate star clusters, bright galaxies, the Moon and planets are easily distinguishable in this aperture size. These models make for great “leave in the car” telescopes so you always have optics at hand. For teens who are interested in astronomy, binoculars make an incredible “First Telescope”. Considering a model in this size will allow for most types of astronomical viewing and with care will last through a lifetime of use.

Binoculars any larger than 50-60mm are some serious aperture. These are the perfect size allowing for bright images at high magnification. For astronomy applications, binoculars with equations like 15X70 or 20X80 are definitely going to open a whole new vista to your observing nights. The wide field of view allows for a panoramic look at the heavens, including extended comet tails, large open clusters such as Collinder Objects, starry fields around galaxies, nebulae and more… If you have never experienced binocular astronomy, you’ll be thrilled at how easy objects are to locate and the speed and comfort at which you can observe. A whole new experience is waiting for you!

Binocular Magnification
When choosing binoculars for astronomy, just keep in mind that all binoculars are expressed in two equations – the magnifying power X the objective lens size. So far we have only looked at the objective lens size. Like a telescope, the larger the aperture, the more light gathering power – increasing proportionately in bulk and weight. Stereoscopic views of the night sky through big binoculars is an incredible, dimensional experience, but for astronomical applications we need these two numbers to play an important role in determining the exit pupil – the amount of light the human eye can accept. By dividing the objective lens (or aperture) size by the magnifying power you can determine a pair of binoculars exit pupil. Let’s take a look at why that’s important.

How do binoculars magnify? What’s the best magnification to use? What magnifying power do I choose for astronomy? Where do I learn about what magnifying power is best in binoculars? Because binoculars are a set of twin refracting telescopes meant to be used by both eyes simultaneously, we need to understand how our eyes function. All human eyes are unique, so we need to take a few things into consideration when looking at the astronomy binocular magnification equation.

By dividing the objective lens (or aperture) size by the magnifying power you can determine a pair of binoculars exit pupil and match it to your eyes. During the daylight, the human eye has about 2mm of exit pupil – which makes high magnification practical. In low light or stargazing, the exit pupil needs to be more around 5 to be usable.

While it would be tempting to use as much magnification as possible, all binoculars (and the human eye) have practical limits. You must consider eye relief – the amount of distance your eye must be away from the secondary lens to achieve focus. Many high “powered” binoculars do not have enough outward travel for eye glass wearers to come to focus without your glasses. Anything less than 9mm eye relief will make for some very uncomfortable viewing. If you wear eyeglasses to correct astigmatism, you may wish to leave your glasses on while using binoculars, so look for models which carry about 15mm eye relief.

Now, let’s talk about what you see! If you look through binoculars of two widely different magnifying powers at the same object, you’ll see you have the choice of a small, bright, crisp image or a big, blurry, dimmer image – but why? Binoculars can only gather a fixed amount of light determined by their aperture (lens size). When using high magnification, you’re only spreading the same light over a larger area and even the best binoculars can only deliver a certain amount of detail. Being able to steady the view also plays a critical role. At maximum magnification, any movement will be exaggerated in the viewing field. For example, seeing craters on the Moon is a tremendous experience – if only you could hold the view still long enough to identify which one it is! Magnification also decreases the amount of light that reaches the eye. For these reasons, we must consider the next step – choosing the binocular magnification – carefully.

Binoculars with 7X magnifying power or less, such as 7X35, not only delivers long eye relief, but also allows for variable eye relief that is customizable to the user’s own eyes and eyeglasses. Better models have a central focus mechanism with a right eye diopter control to correct for normal right/left eye vision imbalance. This magnification range is great for most astronomy applications. Low power means less “shake” is noticed. Binoculars with 8X or 9X magnification also offer long eye relief, and allows comfort for eyeglass wearers as well as those with uncorrected vision. With just a bit more magnification, they compliment astronomy. Binoculars 10 x 50 magnifying power are a category of their own. They are at the edge of multipurpose eye relief and magnifying power at this level is excellent across all subject matter. However, larger aperture is recommended for locating faint astronomy subjects.

Binoculars with 12-15X magnifying power offer almost telescopic views. In astronomy applications, aperture with high magnification is a must to deliver bright images. Some models are extremely well suited to binocular astronomy with a generous exit pupil and aperture combined. Binoculars with 16X magnification and higher are on the outside edge of high magnification at hand-held capabilities. They are truly designed exclusively as mounted astronomical binoculars. Most have excellent eye relief, but when combined with aperture size, a tripod or monopod is suggested for steady viewing. If you’re interested in varying the power, you might want to consider zoom binoculars. These allow for a variety of applications that aren’t dependent solely on a single feature. Models can range anywhere from as low as 5X magnification up to 30X, but always bear in mind the higher the magnification – the dimmer the image. Large aperture would make for great astronomy applications when a quick, more magnified view is desired without being chained to a tripod.

Other Binocular Features
The next thing to do is take a good look at the binoculars you are about to purchase. Check out the lenses in the light. Do you see blue, green, or red? Almost binoculars have anti-reflection coatings on their air to glass surfaces, but not all are created equal. Coatings on binocular lenses were meant to assist light transmission of the object you’re focusing on and cancelling ambient light. Simply “coated” in the description means they probably only have this special assistance on the first and last lens elements – the ones you’re looking at. The same can also be said of the term “multi-coated”, it’s probably just the exterior lens surface, but at least there’s more than one layer! “Fully coated” means all the air-to-glass surfaces are coated, which is better… and “fully multi-coated” is best. Keeping stray light from bouncing around and spoiling the light you want to see is very important, but beware ruby coated lenses… These were meant for bright daylight applications and will rob astronomical binoculars of the light they seek.

Last, but not least, is a scary word – collimation. Don’t be afraid of it. It only means the the optics and the mechanics are properly aligned. Most cheap binoculars suffer from poor collimation, but that doesn’t mean you can’t find an inexpensive pair of binoculars that are well collimated. How can you tell? Take a look through them with both eyes. If you can’t focus at long distance, short distance and a distance in-between, there is something wrong. If you can’t close either eye and come to focus with the other, there’s something wrong. Using poorly collimated binoculars for any length of time causes eye strain you won’t soon forget.

Price range for Astronomy Binoculars
So, how much? What does a good pair of binoculars for astronomy cost? First look for a quality manufacturer. Just because you’ve chosen a good name doesn’t mean you’re draining your pocket. Smaller astronomy binoculars of high quality are usually around or under $25. Mid-sized astronomy binoculars range from $50 to $75 as a rule. Large astronomy binoculars can run from a little over $100 to several hundred dollars. Of course, choosing a high-end pair of binoculars of any size will cost more, but with proper care they can be handed down through generations of users. Keep in mind little things that might be good for your applications, like rubber-coated binoculars for children who bang them around more, or fog-proof lenses if you live in a high humidity area. Cases, lens caps and neck straps are important, too.

Some Suggested Binoculars
The purpose of this guide was to help you understand how to choose the best binoculars for astronomy. But if you trust me, and just want some suggestions… here you go.

For all purpose astronomy binoculars, I’d recommend the Celestron Up-Close and Ultima Series as well as Meade Travel View. Nikkon and Bushnell binoculars in this size range are an investment, and best undertaken after you decide if binocular astronomy and this size is right for you. Amazon.com offers a wide range of these binoculars.

While so much information on binoculars may seem a little confusing at first, just a little study will take you on your way to discovering astronomy binoculars that are perfect for you!

Universe Today Exclusive – Cygnus Nova V2491 Revealed for Readers

Clouds got you down? No chance of seeing V2491 Cyg because of the weather? Are you sleeping when Cygnus is up? One of the most beautiful facets of having an astronomer around is being able to share information with other observatories around the world and put them to work. This time the job was handed to our friends in Australia who were able to produce for us an exclusive look at an elusive nova.

In trial test on image acquisition utilizing the combined resources of Macedon Ranges Observatory and its resident astronomers, they were able to nab the nova in less than 30 minutes from notice being given. The image was then processed, labeled and returned again halfway around the world within hours for UT readers to enjoy.

On 15 April 2008 from 10.50 to 11.40 UT, Joseph Brimacombe from Cairns, Queensland, Australia was busy employing remote technology located at 32 degrees 54 minutes North; 15 degrees 32 min West and recording the nova with an SBIG ST-L-1001 CCD camera. Coupled with a 20″ Ritchey-Chretien Optical System, 8 separate exposures of 5 minutes duration were taken in white light, and the results speak for themselves.

By comparing the zoom map of the area presented in the original Cygnus Nova Alert it’s easy to see the identifying line of three stars which helps orient the viewer to the general area. As predicted, Cygnus Nova V2491 easily stands out amongst the background stars.

Says Observatory Director, Burt Candusio: “The exercise was primarily designed to test the imaging and response capabilities of M.R.O resident astronomers. If another similar event presents itself, we would now be confident in our capabilities of imaging a target effectively and quickly from any part of the globe. A most pleasing outcome for all concerned and especially for Joseph Brimacombe.”

But the thrill was nothing compared to Joe’s own success: “Trapped under the mostly cloudy Cairns skies, I was remotely imaging the running chicken nebula (NGC 2944) at the Macedon Range Observatory and the Pinwheel galaxy (M101) at New Mexico Skies, when my good mate Bert Candusio notified me of a new nova (V2491) in Cygnus. At the time, it was 60 degrees below the horizon at the MRO, but 50 degrees above the horizon at NMS, so I slewed my 20 inch RCOS at NMS to the co-ordinates Bert had provided. There was just sufficient time before dawn to snap 8 x 5 min luminance frames of a dense star field. Both Bert and I were delighted to find the nova near the middle of the frame. We estimate the magnitude at around 10. The beauty of NGC 2944 and M101 was not a match for the excitement of imaging an acute stellar explosion for the first time!”

In the case of V2491 Cyg, the only thing better than having the stars up above is having friends down under. Our thanks go to our friends at Macedon Ranges Observatory!