Green Laser Pointers – Just Mind Your Manners…

Are you among the thousands of amateur astronomers who received a green laser pointer for Christmas and are a bit afraid to take it out of the box? Do the words “You’ll put your eye out.” ring in your head? Like you, I have a green laser pointer… and I’ve accidentally shot myself in the eye. To make matters worse, I’ve even had others inadvertently use my retina as a target. Have I gone blind yet?

The answer is no. But I have gotten a nasty headache and had the “flash bulb” effect for a few hours. It’s true that green lasers aren’t toys, but the reality check is that you really need to mind your manners when using one. “With respect to direct personal danger, potential damage to vision is the only real consideration – there is no risk from radiation or enough power in a beam of less than 5 mW to burn anything. However, from a public policy and regulatory perspective, there are actually three areas of concern.” says Samuel M. Goldwasser. “One – Flash blindness from momentary exposure or permanent damage to vision from prolonged intentional misuse. Laser pointers are usually rated Class IIIa or less which means that the power is low enough that the eye should be protected from permanent damage by natural pupil contraction, blink, and aversion reflexes. Two – Distraction and collateral damage – you wreck your car because someone pointed a laser pointer at you while you were driving. Three – Misinterpretation of intent – you get blown away by someone with a BIG gun who thinks you are targeting them with a laser sight. Or, you are arrested and thrown in the slammer for aiming a laser pointer at a cop (this happened recently).

As Sam’s fine article on Laser Safety goes on to point out: “While I absolutely agree that intentionally aiming a laser of any kind into someone’s eye is basically stupid (unless you are having laser eye surgery), one must be careful in interpreting the meaning of press reports that describe momentary exposure to the beam from a laser pointer waved around an auditorium resulting in instant total loss of vision in all three eyes. One would have to direct the beam into the pupil of the eye from a close distance for a few seconds or more without either the eye or pointer moving, twitching, or blinking. Distance is significant both because even laser pointer beams diverge (especially cheap ones) so less energy is able to enter the pupil of the eye as the source moves further away and it is harder/less likely for it to remain stationary and centered on such a target a few mm across. This is not really possible by accident and even takes significant effort to do intentionally since the eye’s natural pupil contraction, blink, and aversion reflexes will prevent the beam from focusing on a single spot on the retina with a sufficient concentration of energy for more than an instant – not enough time for damage to result. There would have to be cooperation which can only really happen in a game of chicken – but it is hard to protect people from their own stupidity. This does mean, however, as if it isn’t already obvious, that laser pointers should be kept from infants – period, and away from children unless adequately supervised. Adults, on the other hand, presumably know not to stare into painfully bright lights and some may even read the warning labels!”

When it comes to green laser pointers, just remember to mind your manners. Accidentally getting “flashed” – or flashing someone else will make you look like one of the most horribly irresponsible astronomers known to mankind. Using a green laser pointer at a star party when someone is doing long exposure deep sky photography might also result in getting your tripod wrapped around your neck. At the same time, responsible use of a green laser pointer gives you an invaluable educational tool that’s as impressive as it is useful.

Just mind your manners…

If you’d like to know more about lasers and safety – from simple barcode scanners to your CD player and more – please visit Samuel M. Goldwasser’s Laser Safety pages. Also, many thanks to the HoTech Corporation for use of the photos.

Total Lunar Eclipse Information – December 21, 2010

Are you ready? As promised, here comes more detailed information on the 2010 total lunar eclipse. Step inside and find out where and when to watch!

The eclipse begins for eastern North America on Tuesday morning, Dec. 21st, at 1:33 am EST and occurs on Monday night, Dec. 20th, at 10:33 pm PST for western North America. At that time, Earth’s shadow will appear as a dark-red crescent at the edge of the lunar disk. It takes about an hour for the Earth’s shadow to fully encompass the visible side of the Moon. Totality commences at 02:41 am EST (11:41 pm PST) and lasts for 72 minutes. Western Europe and the northwestern portion of Africa will also be treated to a portion of the eclipse at moonset. The point of deepest shadow will occur at 08:17 UT and totality ends 36 minutes later at 08:53 UT. At that time, a silver sliver will once again appear along the lunar limb, where for one hour and eight minutes it will continue until the Moon passes out of the umbral shadow at 10:01 UT. From there it will pass into the penumbral shadow for an additional hour and four minutes until the show ends at 11:05 UT.

Where will the Moon appear? Of course it will be along the ecliptic plane and in very good company – riding high above Orion. Be sure to look for a triple red treat as the show forms a triangle with blushing Betelgeuse and ruddy Aldebaran. As the Moon darkens, be sure to look for wonderful unaided eye deep space objects you can’t see during a full Moon – like the Plieades (M45) and the Great Orion Nebula (M42). What a Christmas treat!

Photographing or videotaping a total lunar eclipse is quite easy, but remember if you live in a cold climate that there are a few very important rules to follow. Number one is to be sure to protect your hands. It’s very easy to get involved with the equipment and ignore what seems like a slight discomfort. You don’t want to experience freezing your fingers to a metal surface or risking frostbite! The second rule is to remember that cold batteries drain very, very quickly. You can easily avoid frustration by simply keeping spares somewhere handy next to your skin. Of course, getting to them might be a ticklish situation! The last rule to remember is simply to dress for success. Multiple loose layers of clothing, hat, gloves and proper footgear are a must where the winter season means bitter cold temperatures.

Now all that’s left is just to let the hours count down… and enjoy!

Fun Facts from NASA: This lunar eclipse falls on the date of the northern winter solstice. How rare is that? Total lunar eclipses in northern winter are fairly common. There have been three of them in the past ten years alone. A lunar eclipse smack-dab on the date of the solstice, however, is unusual. Geoff Chester of the US Naval Observatory inspected a list of eclipses going back 2000 years. “Since Year 1, I can only find one previous instance of an eclipse matching the same calendar date as the solstice, and that is 1638 DEC 21,” says Chester. “Fortunately we won’t have to wait 372 years for the next one…that will be on 2094 DEC 21.”

Total Lunar Eclipse – December 21, 2010

Both lunar and solar eclipses can only occur when the Earth, Sun and Moon are directly aligned… and that alignment is about to happen just four days before Christmas! While the winter treat of totality will lend itself to North America, many other parts of the world will be able to enjoy a partial eclipse as well. Just remember your time zones and I’ll post specific times and locations just a little closer to the date. Right now, let’s learn more!

What is a partial eclipse or totality? When the Earth’s shadow engulfs the Moon, it is a lunar eclipse which occurs in two phases. The outer shadow cone is called the penumbra and the dark, inner shadow is called the umbra. A round body, such as a planet, casts a shadow “cone” through space. When it’s at Earth, the cone is widest at 13,000 kilometers in diameter, yet by the time it reaches the Moon it has narrowed to only 9,200 kilometers. Considering the distance to the Moon is 384,401 kilometers, that’s hitting a very narrow corridor in astronomical terms!

As a rule of thumb, remember that the Moon moves about its own diameter each hour, so the very beginning of a penumbral eclipse will be difficult to notice. Slowly and steadily, the coloration will begin to change and even inexperienced eclipse watchers will notice that something is different. The Moon will never completely disappear as it passes through the Earth’s umbral shadow cone, either. Thanks to our atmosphere bending the sunlight around us, it scatters the light and refracts the signature red and copper coloration we associate with lunar eclipse. Why? Just the small particles in our air – dust and clouds – the shorter wavelengths of light from the Sun are more likely to be scattered (in this case, red) and that’s what we see. Exactly the same reason sunset and sunrise appears to be red! If you’d like to dedicate a portion of your mind to science, then try judging the eclipse coloration on the Danjon scale. It was was devised by Andre Danjon for rating the overall darkness of lunar eclipses:

L=0: Very dark eclipse. Moon almost invisible, especially at mid-totality.
L=1: Dark Eclipse, gray or brownish in coloration. Details distinguishable only with difficulty.
L=2: Deep red or rust-colored eclipse. Very dark central shadow, while outer edge of umbra is relatively bright
L=3: Brick-red eclipse. Umbral shadow usually has a bright or yellow rim.
L=4: Very bright copper-red or orange eclipse. Umbral shadow is bluish and has a very bright rim.

Now we know what to plan for! Time to get your winter gear ready. Photographing or video taping an eclipse is easy – but remember if you live where it is very cold that your batteries will expire fast – so keep an extra set in a warm place next to your body.

Be sure to check back for specific times and locations here at UT on December 20th… and tell your family and friends about the very special Christmas present that’s coming your way!

Eclipse Images Courtesy of Doug Murray (top), Tom Ruen (bottom) and NASA (center illustration). We thank you!

Red Sky In The Morning…

“Red sky in the morning… Sailors take warning!” How many of you have heard of that old phrase? Just look at this beautiful panorama of Cairns, Australia done by Joe Brimacombe – does it portend foul weather ahead or are such sayings a myth? Step inside and let’s find out…

In present time we recognize such beautiful clouds to be a reflection from the rising Sun, but in times past mankind relied on such fanciful wordsmithing to help them predict weather patterns crucial to farmers and sailors. Can the appearance of the sky and appearance of the clouds really foretell the atmospheric future? You just might be surprised…

Generally our weather moves in the opposite direction – west to east – from which our Earth turns. It’s carried along by the romantic westerly trade winds, meaning storm systems are more likely to arrive from the west. We know the brilliant and varied colors we see in the sky are caused by sunlight being refracted into almost all the colors of the spectrum as they pass through our atmosphere and bounce off the water vapor and fine particles present in Earth’s atmosphere. The amount, of which, are darn good indications of weather-to-be!

At both rise and set, the Sun is low on the horizon and the light coming through is penentrating the very thickest part of Earth’s atmosphere. When skies appear red, we know it carries a concentration of both moisture and dust particles. We perceive red because the longest wavelengths in the visible spectrum dictate it. The shorter blue wavelengths are dispersed. Therefore a red sunrise means the Sun is reflecting from dust particles and clouds that have passed from the west and a storm may be following in from the east. Watch for the skies themselves to change color, too… Because if they should appear a deep, brilliant red? That means there’s a high moisture content in the atmosphere and rain is usually on the way!

And now you know…

Many thanks to Dr. Joseph Brimacombe for sharing his awesome photo taken from Coral Towers Observatory, Cairns, Australia. You rock, Doc!

The Lion Tamer – Leonid Meteor Shower 2010

Are you ready to walk into the lion’s cage? Then break out your favorite skywatching gear because the 2010 Leonid meteor shower is underway…

In the pre-dawn hours on the mornings of November 17 and November 18, the offspring of Comet Temple/Tuttle will be flashing through our atmosphere and just taunting you to test your meteor watching skills against bright skies. Although the phat Moon will greatly interfere with fainter meteor trails, don’t let that stop you from enjoying your monring coffee with the sparkling “cubs” that will be shooting out from the constellation of Leo.

Where? For all observers the constellation of Leo is along the ecliptic plane and will be near its peak height during best viewing times. When? Because of the Moon, just a couple of hours before local dawn is the best time to watch. Why? Read on!

Although it has been a couple of years since Temple/Tuttle was at perihelion, don’t forget that meteor showers are wonderfully unpredictable and the Leonids are sure to please with fall rate of around 20 (average) per hour. Who knows what surprises it may bring! Each time the comet swings around our Sun it loses some of its material in the debris trail. Of course, we all know that is the source of a meteor shower, but what we don’t know is just how much debris was shed and where it may lay.

As our Earth passes through the dusty matter, it may encounter a place where the comet let loose with a large amount of its payload – or it may pass through an area where the “comet stuff” is thin. We might even pass through an area which produces an exciting “meteor storm” like the Leonids produced in 1883! For those in the know, the Leonid meteor shower also made a rather incredible appearance in 1866 and 1867 – dumping up to 1000 (not a typo, folks) shooting stars recorded even with a Moon present! It erupted again in 1966 and in 1998 and produced 3000 (yep. 3000!) video recorded meteors during the years of 2001 and 2002. But remember, human eyes may only be able to detect just a few…

And I ain’t lion!

Photo Courtesy of Stardate.org, Texas University

Dances With Comets – C/2010 V1 Ikeya Murakami

For those of you working on your Comet Hunter’s certificates – or for those who just love these travelers from the Oort Cloud – there’s a new partner in the morning sky. Say hello to C/2010 V1 Ikeya Murakami! If you’re familiar with how a comet looks and already know the steps, then let the easiness lure you out. However, if you’ve never danced with a comet before, then come inside and we’ll teach you the steps…

Our first teacher is John Chumack of Galactic Images who sent us the lead picture for this article. Not all comets jump right out of the sky at you, and some require you wait for just the precise moment in time to catch it. As John says, “I had a very short window to grab it. I could not take more shots due to Dawn rising fast! But I did get very nice details… and it is sporting a little red tail, and a great bow shock!” As you can read, even just a few moments are worth it and the clue here is that Comet Ikeya Murakami isn’t in the easiest of places for most observers. How about if we find out exactly where to look?

Follow the green brick road! This morning comet Ikeya Murakami would have been a same field object with Saturn and it’s headed toward Venus. How easy can it get? Simply aim your binoculars at Saturn and slowly follow the trajectory towards Venus. By November 30 Ikeya Murakami will be about 2 degrees north of the stunningly bright planet and also a same field object in most binoculars.

So, what would the comet be like to watch for awhile? First off, remember that what you will see in binoculars and a small telescope will resemble a small, unresolved globular cluster. It will be a faint fuzzy with a faint tail. More aperture will help, but the approaching Sun is the real culprit here. Comet C/2010 V1 Ikeya Murakami won’t be terribly bright, but you might catch other interesting things while you watch, too. Just ask the one and only Joe Brimacombe!

If you don’t catch C/2010 V1 Ikeya Murakami on the first try – don’t be disappointed… And try again! (the “Aqua” Man would.) But don’t wait too long because the Moon is going to be along soon, making morning skies even brighter. If you do catch it, be sure to share your impressions with us…

Cuz’ there ain’t nothin’ like a little dance before dawn.

New Supernova Lights Up Leo

A new supernova? Darn right. Lighting up Leo? Well… not without some serious visual aid, but the fact that someone out there is watching and has invited us along for the ride is mighty important. And just who might that someone be? None other than Tim Puckett.

Less than 24 hours ago, the American Association of Variable Star Observer’s Report #222 stated:

“Bright Supernova in UGC 5189A: SN 2010jl
November 5, 2010

We have been informed by Tim Puckett and by the Central Bureau for Astronomical Telegrams (CBET 2532, Daniel W. E. Green, Ed.) of the discovery of a bright supernova in UGC 5189A by J. Newton and Puckett, Portal, AZ, on November 3.52 UT at unfiltered magnitude 13.5. Confirming images (limiting magnitude 19.1) by Puckett on Nov. 4.50 UT showed the object at magnitude 12.9.

Spectroscopic observations (CBET 2536, Daniel W. E. Green, Ed.) by S. Benetti and F. Bufano, Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Padova, on behalf of a larger collaboration, and by J. Vinko, University of Szeged, G. H. Marion, Harvard-Smithsonian Center for Astrophysics and University of Texas, T. Pritchard, Pennsylvania State University, and J. C. Wheeler and E. Chatzopoulos, University of Texas, show that SN 2010jl is a type-IIn supernova. Vinko et al. also report that simultaneous measurements with Swift/UVOT in the ultraviolet bands confirm that the transient is ultraviolet-bright, as expected for young, interacting supernovae.

Coordinates: 09 42 53.33 +09 29 41.8 (J2000.0) This position is 2.4″ east and 7.7″ north of the center of UGC 5189A. This AAVSO Special Notice was prepared by Elizabeth O. Waagen.”


While magnitude 12-12.9 isn’t unaided eye bright by a long shot, it’s well within the reach of most of today’s backyard telescopes. The image you see here on the right is of UGC 5189A before the event and the lefthand image was taken at the time of the supernova report. Visually the SN event outshines the galaxy! While chasing a faint supernova event might not be everyone’s cup of tea, Mr. Puckett’s devotion is absolutely legendary and I strongly encourage you to have a look if you have the the tools and talent.

So many supernovae… So little time!

Jupiter Makes Close Pass At Earth…

Image Credit: Babak A. Tafreshi

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Look! Up in the sky! Is it a bird? Is it a plane? No… It’s super Jupiter! “Jupiter is always bright, but if you think it looks a little brighter than usual this month, you’re right,” says Robert Naeye, editor in chief of Sky & Telescope magazine. “Jupiter is making its closest pass by Earth for the year. And this year’s pass is a little closer than any other between 1963 and 2022.”

Where do you find Jupiter? Try about 368 million miles away and (for most observers) low to the southeast after the skies get dark. The giant planet will reach its nearest point to us on the evening of September 20, 2010 – but will remain one of the brightest objects in the night through the end of the month.

Why does Jupiter appear to be more luminous now than at any other time? Although the varying distances over the years may seem marginal – about 10 to 11 million miles over a period of around 60 years – it translates into significance when it comes to magnitude factors. At its brightest, Jupiter can reach –2.94, and dimmest at -1.6. Just a 1% distance change can mean either 4% brighter or dimmer!

The mighty Jove has also undergone some cosmetic changes in the past year as well, making it an additional 4% brighter than usual.

For nearly a year the giant planet’s South Equatorial Belt has slowly been covered by a highly reflective ammonia cloud. Normally the SEB appears to be brown, a result of Jupiter’s chemical compounds reacting to the Sun’s ultraviolet light. Known as “chromophores”, these chemicals are known to mix with lower cloud decks and just a few stormy days could mean rising convection cells are forming crystallized ammonia – masking the light absorbing dark zone and adding to reflectivity.

Of course, a close pass doesn’t mean Jupiter is going to appear to be the size of the Moon – nor be as bright – but it’s certainly going to make a grand appearance on the nights of September 22 and September 23 when it joins Selene on the celestial scene!

But that’s not all that’s happening here. According the Sky & Telescope Magazine: Jupiter and Uranus find themselves close to the point on the sky known as the vernal equinox, where the Sun crosses the celestial equator on the first day of spring. (“Spring” here means spring in the Northern Hemisphere.) And, all of this takes place around the date when fall begins in the
Northern Hemisphere: on September 22nd. (Fall begins at 11:09 p.m. Eastern Daylight Time on that date.)

What do all these coincidences mean? “Nothing at all,” says Alan MacRobert, a senior editor at Sky & Telescope. “People forget that lots of things are going on in the sky all the time. Any particular arrangement might not happen again for centuries, but like the saying goes, there’s always something. Enjoy the show.”

Image Credits In Order of Appearance: Babak A. Tafreshi, Sky & Telescope magazine / Sean Walker and visualization courtesy of Sky & Telescope magazine.

Step On The Scales: Weighing Up Planet Earth…

Scientists at the European Southern Observatory have identified the closest looking solar system to our own. They located a sun-like star more than 100 light years distant with as many as seven different planets, including one that might be the smallest ever found outside the solar system.

“We have found what is most likely the system with the most planets yet discovered,” says Christophe Lovis, lead author of the paper reporting the result. “This remarkable discovery also highlights the fact that we are now entering a new era in exoplanet research: the study of complex planetary systems and not just of individual planets. Studies of planetary motions in the new system reveal complex gravitational interactions between the planets and give us insights into the long-term evolution of the system.”

Some of the planets identified are large but one is only 1.4 times the size of Earth. That’s getting tantalizingly close to finding what astronomers are calling the ‘Holy Grail’ of astronomy, locating a planet just like our own with a breathable atmosphere, moderate temperatures and orbital stability. Scientists have been spotting planets beyond our solar system for the past 15 years, and they’ve now cataloged some 450. They know there are many more out there. The newly found worlds are made essentially of rocks and ice with a solid core. The larger planets probably have a layer of hydrogen and helium gas like Uranus and Neptune and the sixth is possibly a Saturn-like planet.

“We also have good reasons to believe that two other planets are present,” says Lovis. One would be a Saturn-like planet (with a minimum mass of 65 Earth masses) orbiting in 2200 days. The other would be the least massive exoplanet ever discovered [2], with a mass of about 1.4 times that of the Earth. It is very close to its host star, at just 2 percent of the Earth–Sun distance. One “year” on this planet would last only 1.18 Earth-days.

“This object causes a wobble of its star of only about 3 km/hour — slower than walking speed — and this motion is very hard to measure,” says team member Damien Ségransan. If confirmed, this object would be another example of a hot rocky planet, similar to Corot-7b.

Since the Earth is suspended in space, it cannot be put on a scale and weighed to be compared to other planets. But scientists can estimate its total weight by, among other things, measuring its tug on orbiting satellites. We’ve used this method to weigh the Earth and it turns out to be a whopping 6.6 sextillion tons… that’s two 6s, followed by twenty zeros, or 6,600,000,000,000,000,000,000 tons! But Earth’s weight gain doesn’t stop there… it increases by 100,000 pounds each year from dust and meteoric material falling from the sky. How does this “weigh up” to planetary science?

“Clearly, the exploration of the low-mass planet population has now fully started,” says C. Lovis et al. “The HARPS search for southern extra-solar planets will become the main focus of the field in the coming years. It is expected that the characterization of planetary system architectures, taking into account all objects from gas giants to Earth-like planets, will greatly improve our understanding of their formation and evolution. It will also allow us to eventually put our Solar System into a broader context and determine how typical it is in the vastly diverse world of planetary systems. The characterization of a significant sample of low-mass objects, through their mean density and some basic atmospheric properties, is also at hand and will bring much desired insights into their composition and the physical processes at play during planet formation.”

Many thanks to Dave Reneke of Australasian Science Magazine for sharing and to Mission Green Globe and ESO for the images.

Ars Electronica Festival – Don’t Miss September 6!

Ars Electronica made its debut on September 18, 1979. This festival of art, technology and society spotlighted the emerging Digital Revolution. In his preface to what was going on then, Mayor Franz Hillinger wrote (with specific reference to music): “Ars Electronica is giving rise to a new tonal coloration in which state-of-the-art technology is dovetailing with the intellectual spirit of the age to open up undreamt-of expressive possibilities. […] I am absolutely convinced that this new melodic parlance will ultimately be widely understood. After all, with the help of electronic music, it can even be made visible, be implemented in color, contour, line and rhythm that can be followed onscreen.” He would be proven correct.

Within a few years, Ars Electronica developed into one of the world’s foremost media art festivals. And its growing success was paralleled by the expansion of its annual lineup of events. The 1979 festival proudly presented 20 artists and scientists; in 2008, no fewer than 484 speakers and artists from 25 countries were in attendance. Don’t miss this year’s Live Stream on September 6 at 14:00 UT!

For more than three decades now, this world-renowned event has provided an annual setting for artistic and scientific encounters with social and cultural phenomena that are the upshot of technological change. Symposia, exhibitions, performances and interventions carry these inquiries beyond the confines of conventional conference spaces and cultural venues and take them out into the public sphere and throughout the cityscape. In this process of pervading public spaces and staging festival activities in interesting and appropriate physical settings, Ars Electronica has consistently displayed extraordinary imaginativeness. From the harbor to the mines, from factories to outlying monasteries, unusual locations have repeatedly served as sites of performances and interventions, and have, in turn, been reinterpreted by them.

But the attractiveness of Ars Electronica isn’t attributable solely to participation by renowned scientists and artists from all over the world. Or to remarkable venues. Above all, it’s the international audience that makes the biggest contribution to the festival spirit: the colorful mix of old friends and new faces who conjure up extraordinary circumstances – a “fruitful state of emergency” – every September in Linz.

Be sure to tune in on Monday, September 6th when the Ars Electronica Festival will be featuring Repair dealing with the issues of light pollution!

Orignal Source: ARS Electronica