Meteor Showers Archives

December 9, 2013December 23, 2015 by David Dickinson

Get Ready for the 2013 Geminid Meteor Shower

The rising radiant of the Geminids-Looking east at 9PM local from latitude 30 degrees north. (Credit-Stellarium).

One of the best annual meteor showers occurs this coming weekend.

The 2013 Geminid meteors peak this coming Saturday on December 14^th. This shower has a broad maximum, assuring that observers worldwide get a good look. In 2013, the maximum for the Geminids is forecast to span from 13:00 Universal Time (UT) on Friday, December 13^th to 10:00UT/5:00AM EST on Saturday, December 14^th, with a projected maximum centered a few hours earlier at 2:00 UT Saturday morning.

This is good news for observers spanning both sides of the Atlantic, who should be well placed to catch the event. Keep in mind, meteor showers often peak hours before or after predictions… we certainly don’t know everything that a given meteor stream might have in store!

An all-sky composite of the 2008 Geminid meteor shower. (Credit: NASA/MSFC/Bill Cooke, NASA's Meteoroid Environment Office). — An all-sky composite of the 2008 Geminid meteor shower. (Credit: NASA/MSFC/Bill Cooke, NASA’s Meteoroid Environment Office).

But the time to start watching is now. We’ve already seen a few early Geminids this past weekend, and this shower is notable for showing early activity for northern hemisphere observers before local midnight. This is because the radiant, or the direction that the meteors seem to emanate from lies at a high northern declination of 33 degrees north near the star Castor, also known as Alpha Geminorum.

The typical Zenithal Hourly Rate for the Geminids is 80-120, or about 1 to 2 per minute. Keep in mind, the ZHR is an ideal rate, assuming dark skies, with the radiant positioned directly overhead. Most observers will see significantly less activity.

The 2013 Geminids also have to contend with the waxing gibbous Moon, which reaches Full just 3 days after the shower’s expected maximum. This will give observers a dwindling window between moonset and the start of dawn twilight to catch the Geminids at their best.

We always thought that the Geminids had a bit of an undeserved PR problem among annual showers. This no doubt stems from the fact that they arrive in the chilly month of December, a time when fingers go numb, camera batteries die, and conducting a vigil for meteors is challenging.

A 2012 Geminid captured by the author from Mars Hill. North Carolina. — A 2012 Geminid captured by the author from Mars Hill, North Carolina.

This shower is an interesting one though, with an equally interesting history and source. The Geminids were first identified as a distinct meteor shower by R.P. Greg of Manchester UK in 1862, and the estimated ZHR rose from about 20 to 80 through the 20^th century. The parent source of the Geminids remained unknown until 1983, when astronomer Fred Whipple linked them to the strange “rock-comet” body 3200 Phaethon. An Apollo asteroid also thought to be a member of the Pallas family of asteroids, 3200 Phaethon seems to be shedding enough material to produce the annual Geminid meteor shower. This makes the annual shower rare as one not produced by a comet. It’s worth noting that 3200 Phaethon also passes extremely close – 0.14 AU – from the Sun at perihelion, and gets periodically “baked” during each 1.4 year passage.

In the 21^st century, rates for the Geminids have stayed above a ZHR of 120, currently the highest of any annual shower. It’s worth noting that an extrapolated ZHR of almost 200 were seen in 2011 when the Moon was at an equally unfavorable waning gibbous phase! The Geminids always produce lots of fireballs, capable of being seen even under moonlit skies.

There are also two other showers currently active to watch for this week. One is the Ursid meteors, which radiate from the Little Dipper (Ursa Minor) with a peak ZHR of 10-50 occurring on December 22^nd. Also, keep an eye out for Andromedid meteors this week, a defunct shower that may be making a comeback. The source of several great meteor storms in the late 19^th century, the Andromedid parent source is the shattered comet formerly known as 3D/Biela.

An early Geminid crosses pathes with Comet 2013 R1 Lovejoy. (Credit: Jason Hullinger). — An early Geminid crosses paths with Comet 2013 R1 Lovejoy. (Credit: Jason Hullinger).

Though the Geminids appear to radiate from the constellation Gemini, they can appear anywhere in the sky. Tracing the path back can determine the source constellation and the “membership” of a given meteor. Random meteors not associated with any identified shower are known as “sporadics.” Block that pesky light-polluting Moon behind a building or hill to optimize your chances of catching sight of a meteor. Employing a friend or two to watch in different directions will also maximize the number seen. The International Meteor Organization always welcomes reports from observers… this is real science that you can contribute to using nothing more sophisticated than your eyes!

The Geminids are medium-speed meteors with an average atmospheric velocity of about 35 kilometres per second, often leaving long, glowing trails worth examining with a pair of binoculars. You might note an apparent surge in speed to this shower past local midnight, as your vantage point turns into the oncoming shower, adding the velocity of the Earth to the approaching Geminids.

Photographing meteors is fun and easy to do; all you’ll need is a DSLR camera mounted on a tripod. Take several manual setting exposures to get the combination of ISO,F-stop, and shutter speed correct for your local sky conditions. Then simply set the focus to infinity, and use the widest field of view possible. Catching meteors is surreptitious, as they can appear anywhere – and at any time – in the sky. Be sure to thoroughly review those images afterwards… nearly every meteor we’ve caught photographically went unnoticed during observation!

Also, remember that cold weather plus long exposure times can conspire to drain camera batteries in a hurry. Be sure to keep a spare set of charged batteries ready to go in a warm pocket!

How powerful will the Geminids become? Are we in for a “return of the Andromedids” moving towards 2014? One thing is for sure: you won’t see any meteors if you don’t try. So be sure to get out there, pour a mug of your favorite warming beverage, and don’t miss the 2013 Geminid meteor shower!

– Got meteors? Be sure and tweet ‘em to #Meteorwatch.

– Be sure to send those pics of Geminids and more in to Universe Today.

November 14, 2013December 23, 2015 by David Dickinson

Here Comes the Weekend Leonid Meteor Shower!

November 2013 offers a chance to catch a dependable meteor shower, albeit on an off year. The Leonid meteors are set to reach their annual peak this coming weekend on Sunday, November 17th. We say it’s an off-year, but not that it should discourage you from attempting to catch the Leonids this weekend in the early dawn.

Projections for 2013 suggest a twin-peaked maximum, with the first peak arriving on November 17^th at 10:00 UT/5:00 AM EST favoring North America, and the second one reaching Earth on the same date six hours later at 16:00 UT/11:00, favoring the central Pacific.

Unfortunately, the Full Moon also occurs the on very date that the Leonids peak at 10:16 AM EST/ 15:16UT, right between the two peaks! This will definitely cut down on the number of meteors you’ll see in the early AM hours.

That’s strike one against the 2013 Leonids. The next is the curious sporadic nature of this shower. Normally a minor shower with a zenithal hourly rate (ZHR) in the range of 10-20 per hour, the Leonids are prone to great storms topping a ZHR of 1,000+ every 33 years. We last experienced such an event in 1998 and 1999, and we’re now approaching the mid-point lull between storms in the 2014-2016 time frame.

An early Leonid meteor captured last week from the United Kingdom Meteor Observing Network's Church Crookham station. (Credit: UKMON/Peter-Campbell-Burns). — An early Leonid meteor captured last week from the United Kingdom Meteor Observing Network’s Church Crookham station. (Credit: UKMON/Peter-Campbell-Burns).

Still, this is one shower that’s always worth monitoring. The source of the Leonids is Comet 55p/Tempel-Tuttle, which is on a 33-year orbit and is due to reach perihelion again in 2031.

Note that the Leonids have also continued to show enhanced activity in past years even when the Moon was a factor:

2012- ZHR=47.

2011- ZHR=22, Moon=8% waning gibbous.

2010- ZHR=40, 86% waxing gibbous.

2009- ZHR=79.

2008-70 ZHR=72% waning gibbous

We even managed to observe the Leonid meteors from Vail, Arizona in 2002 and 2005, on years when the Moon was nearly Full.

Now, for the good news. The Leonids have a characteristic r value of 2.5, meaning that they produce a higher than normal ratio of fireballs. About 50-70% of Leonid meteors are estimated to leave persistent trains, a good reason to keep a pair of binoculars handy. And hey, at least the 2013 Leonids peak on the weekend, and there’s always comet’s ISON, X1 LINEAR, 2P/Encke and R1 Lovejoy to track down to boot!

A 2002 Leonid captured over Redstone Arsenal, Alabama. (Credit: NASA/MSFC/MEO/Bill Cooke).

Here’s a few tips and tricks that you can use to “beat the Moon” on your Leonid quest. One is to start observing now, on the moonless mornings leading up to the 17^th. You’ll always see more Leonid meteors past local midnight as the radiant rises to the northeast. This is because you’re standing on the portion of the Earth turning forward into the meteor stream. Remember, the front windshield of your car (the Earth) always collects the most bugs (meteors). Observers who witnessed the 1966 Leonid storm reported a ZHR in excess of thousands per hour, producing a Star Trek-like effect of the Earth plowing through a “snowstorm” of meteors!

The radiant of the Leonids sits in the center of the backwards question mark asterism of the “Sickle” in the astronomical constellation Leo (hence name of the shower).

You can also improve your prospects for seeing meteors by blocking the Moon behind a building or hill. Though the Leonids will appear to radiate from Leo, they can appear anywhere in the sky. Several other minor showers, such as the Taurids and the Monocerotids, are also active in November.

Meteor shower photography is simple and can be done with nothing more than a DSLR camera on a tripod. This year, you’ll probably want to keep manual exposures short due to the Full Moon and in the 20 seconds or faster range. Simply set the camera to a low f-stop/high ISO setting and a wide field of view and shoot continuously. Catching a meteor involves luck and patience, and be sure to examine the frames after a session; every meteor I’ve caught on camera went unnoticed during observation! Don’t be afraid to experiment with different combinations to get the sky conditions just right. Also, be sure to carry and extra set of charged camera batteries, as long exposures combined with chilly November mornings can drain DSLR batteries in a hurry!

A Woodcut print depicting the 1933 Leonids as seem from Niagara Falls. (Wikimedia Commons image in the Public Domian). — A Woodcut print depicting the 1933 Leonids as seem from Niagara Falls. (Wikimedia Commons image in the Public Domain).

The Leonids certainly have a storied history, dating back to before meteors where understood to be dust grains left by comets. The 1833 Leonids were and awesome and terrifying spectacle to those who witnessed them up and down the eastern seaboard of the U.S. In fact, the single 1833 outburst has been cited as contributing to the multiple religious fundamentalist movements that cropped up in the U.S. in the 1830s.

We witnessed the 1998 Leonids from the deserts of Kuwait while stationed at Al Jabber Air Base. It was easily one of the best meteor displays we ever saw, with a ZHR reaching in access of 500 per hour before dawn. It was intense enough that fireballs behind us would often light up the foreground like camera flashes!

Reporting rates and activity for meteor showers is always fun and easy to do — its real science that you can do using nothing more than a stopwatch and your eyes. The International Meteor Association is always looking for current meteor counts from observers. Data goes towards refining our understanding and modeling of meteor streams and future predictions. The IMO should also have a live ZHR graph for the 2013 Leonids running soon.

Have fun, stay warm, send those Leonid captures in to Universe Today, and don’t forget to tweet those meteors to #Meteorwatch!

August 15, 2013December 23, 2015 by Nancy Atkinson

Incredible Footage Shows a Perseid Meteor Exploding

Screen grab from Michael K. Chung's timelapse of a Perseid meteor exploding.

Personally, I’ve never seen anything like this, and photographer and digital artist Michael K. Chung said he couldn’t believe what he saw when he was processing images he took for a timelapse of the Perseid meteor shower. It appears he captured a meteor explosion and the resulting expansion of a shock wave or debris ring.

“It was taken early in the morning on August 12, 2013 from my backyard in Victorville, CA,” Michael told Universe Today via email. “The fade to white is NOT an edit- it is overexposure due to the sun coming up. From what I can tell, the timelapse sequence of the explosion and expanding debris span an actual time of approximately 20 minutes.”

Michael said because he shoots at much higher resolution than 720p, he’s able to provide two different sequences in this video: one is with the full frame of each capture scaled/reduced and then cropped down to 1280×720, and the other is with the full frame kept at resolution with just the region around the explosion cropped to 1280×720. “I included each sequence twice – once at 24 frames per second and the other at around 12 fps.”

Amazing!

Since I’ve never seen anything like this, I decided to have one of our observing experts provide his opinion. UT writer David Dickinson said this is definitely legitimate.

“What cinches it for me is that the meteor was moving in the right direction for a Perseid,” Dave told me. “I see Perseus rising to the right, the plane of the Milky Way and Andromeda just above center.”

Dave said he has seen several meteors that leave lingering smoke trains. “I usually carry binoculars to examine these,” he said, “and saw several examples of this during the 1998 Leonid meteor storm from the desert in Kuwait, one of the most awesome things I’ve seen. Ever.”

Dave concurs, great catch by Michael Chung!

Update: Daniel Fischer provided a link to some imagery and information of the 1998 Leonid observations, showing persistent trains and more. Daniel also provided a more accurate description of what Michael Chung captured: “a persistent train after a Perseids fireball, being torn apart by upper atmosphere wind shear.”

Second update:

We heard from a few more people who also witnessed and captured similar Perseids with persistent trains.

Steve Knight from the UK also captured some explody-Perseids this year. Take a look at his video below, and at :15 and :19 there are fireballs followed by expanding cloud of debris — to see it better expand the video and look at the top right part of the screen. Andromeda Galaxy (M31) is visible drifting in from the left.

And Steve also provided animated gifs of the explosions:

Also, Randy Halverson from Dakotalapse, whose work we feature frequently on UT sent a couple of images of persistent trains from meteors, like this one:

Meteor with persistent train, taken on October 6th, 2012, from the same spot a similar image was taken a year earlier. Credit and copyright: Randy Halverson/dakotalapse.

…and this one of the cloud of debris left from a persistent train:

Cloud of debris from a meteor explosion seen near the White River in South Dakota on October 1, 2011. Credit and copyright: Randy Halverson/dakotalapse.

Watch his timelapse here, with the explosion taking place at about :53 into the film:

… with an interesting story that he set up his equipment to do a timelapse in the same place two years in a row and captured persistent trains both years. To find out more about that, as well as get more info on persistent trains, Phil Plait wrote this article about it.

There’s also an animated gif of an exploding Perseid from astromel on Flickr here.

2013 Perseids Meteor Shower: Meteor Explosion from Michael Chung on Vimeo.

August 14, 2013April 8, 2018 by Nancy Atkinson

Two Beautiful Timelapse Videos of the 2013 Perseid Meteor Shower

Composite image of the Perseid Meteor Shower radiant, from the Mount Lemmon SkyCenter in Arizona. Credit and copyright: Adam Block.

We’re still swooning over the great images and videos coming in from this year’s Perseid Meteor Shower. Here are a couple of timelapse videos just in today: the first is from P-M Hedén showing 25 Perseid meteors, but you can also see Noctilucent clouds, a faint Aurora Borealis, airglow, satellites passing over and lightning. “It was a magic night!,” P-M said.

See another view from the Mount Lemmon SkyCenter in Arizona, below:

This timelapse was created by Adam Block and shows a few hours of the experience guests at the Mount Lemmon SkyCenter had on August 11/12, 2013 during the Perseids: they could look through the 0.8m Schulman telescope and enjoy being outside to see the meteors streaking overhead. Flashlights and other sources illuminate the ground and the observatory. Find out more about the observatory here.

August 12, 2013December 23, 2015 by Nancy Atkinson

Perseid Meteor Shower 2013: Images from Around the World

A composite of stacked images of the Perseid Meteor Shower on August 11, 2013 seen from Lindisfarne (Holy Island) off the northeast coast of England. Credit and copyright: Peter Greig.

The Perseid Meteor Shower peaks tonight, but already astrophotographers have been out, enjoying the view of a little cosmic rain. This weekend provided good views for many, as these images and videos will attest. We’ll keep adding more images as they come in, but enjoy these wonderful images we’ve received so far. Our lead image is a wowza from Peter Greig from the UK. He traveled to an island off the coast of England and found exactly what he was looking for.

“This is the exact image that I imagined and planned to come home with from that trip,” Peter said via Flickr. “It is a composite of stacked images (or pieces of images). I chose the clearest background image to use for the starry sky then chose the best light painted foreground and layered it over my background. I then went through all of my images and gathered all the shots that contained a meteor, cut them out and layered them on top of my background image to demonstrate the radiant point to which the Perseid Meteors originate.”

Just gorgeous! If you’re looking to get out tonight and see the Perseids for yourself, here our “explainer” from David Dickenson of how to best see this meteor shower!

See more from our astrophotographer friends below:

Perseid Meteor and the Milky Way, in the Red Desert of Wyoming, August 11, 2013. Credit and copyright: Randy Halverson/dakotalapse.

Early Perseids from the Washburn-Norlands Living History Center in Livermore, Maine, taken August 5, 2013. Credit and copyright: Steven Coates.

This video is from John Chumack, who captured 142 Perseids from my backyard in Dayton, Ohio! “My video cameras actually caught many more than I had seen visually,” John said via email, expressing a little disapointment in this year’s Persieds, “from past years experiences I was expecting more Perseids!”

A persistent Perseid on August 11, 2013. Shot with Canon T1i/500D with Samyang 8mm fisheye. F5.6 / 3200ISO / 30s. Credit and copyright: darethehair on Flickr.

A very bright fireball from the Perseid meteor shower, along with the Otto Struve Telescope from the McDonald Observatory in Texas and the Milky Way. Credit and copyright: Sergio Garcia Rill/SGR Photography.

You can read more about this image by Sergio Garcia Rill and the ‘persistent’ neon fireball at his website.

A Perseid meteor and the constellation Cassiopeia seen over Winchester, UK. Credit and copyright: Paul Williamson.

Now more:

Can you spot a total of 6 meteors in this image? (two are very faint). This is a composite of 3 pictures stacked, each picture taken with a Canon 550D @18mm 30s Exposure at ISO 3200. Credit and copyright: Andrei Juravle.

2013 Perseids Radiant Point: A composite shot of Perseid meteors emanating from the meteor shower radiant point. This composite features 9 total Perseid meteors. Credit and copyright: Scott MacNeill.

A Perseid meteor and the Milky Way. Credit and copyright: TheMagster3 on Flickr.

Perseid meteor shower (and equipment!) taken on August 11, 2013 near Monte Romano, Lazio, Italy, with a Nikon D5200. Credit and copyright: marcopics3000 on Flickr.

Perseid Meteor Shower and Milky Way image shot in Hampstead, North Carolina on a Canon 7D @10mm 30s f/4 ISO 2500. Credit and copyright: K.C. Goshert.

New images added 8/13/13:

Perseid meteor captured by Emilia Howes, aged 7, at Lacock in Wiltshire, England.

Perseid Meteors over Ancient Bristlecone Pine in the White Mountains of California. This is a composite shot of 73 meteors, aligned as they were captured according to where they were against the stars. Credit and copyright: Kenneth Brandon.

Perseids over Joshua Tree. This is a composite image composed of 180 stills from a static timelapse sequence, aiming towards the North Star. Taken on August 9, 2013. Credit and copyright: Sean Parker/Sean Parker Photography.

'My first-ever photo of a meteor!' said astrophotographer Dawn Sunrise on Flickr. Congrats! — ‘My first-ever photo of a meteor!’ said astrophotographer Dawn Sunrise on Flickr. Congrats!

Perseid meteor photographed on August 11, 2013 at 0255 EDT through broken clouds, Weatherly, PA. 20 second exposure, ISO 1600 using a Samyang 14mm lens. Credit and copyright: Tom Wildoner.

One Perseid meteor before the clouds rolled in over Blackrod, England, August 12, 2013. Credit and copyright: TheDaveWalker on Flickr.

Perseid meteor on August 12, 2013. Credit and copyright: Stephen Rahn.

Perseids Meteor 8/11/2013 El Dorado Lake, Kansas. Credit and copyright: Tom Wright.

More images added 8/15/13:

Meteor seen over Green Bay, Wisconsin on August 14, 2013 around 12:30 am central time. Photographer Michelle Madruga said, 'I used my measly Canon T3i and my 18-55mm lens set at 18mm. During my 30 sec exposure, this huge asteroid shot across the sky! I was lucky it was in my camera's view!' Credit and copyright: Michelle Madruga. — Meteor seen over Green Bay, Wisconsin on August 14, 2013 around 12:30 am central time. Photographer Michelle Madruga said, ‘I used my measly Canon T3i and my 18-55mm lens set at 18mm. During my 30 sec exposure, this huge asteroid shot across the sky! I was lucky it was in my camera’s view!’ Credit and copyright: Michelle Madruga.

Perseid meteor seen over the Rocky Mountains of Colorado, taken with a Canon 7D 18-55mm. Credit and copyright: Micah Holtgraves.

Perseid meteor. Credit and copyright: Val Camp.

Perseid meteor on August 13, 2013 seen over Kootwijkerzand, at the ‘de Hoge Veluwe’, one of the last dark spots in the Netherlands. This picture was taken with an EOS 60d with a 11-16 2.8 tokina lens. Credit and copyright: Freek vd Driesschen.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

August 3, 2013January 22, 2021 by David Dickinson

The 2013 Perseid Meteor Shower: An Observer’s Guide

The radiant for the Persieds, looking to the NE from latitide ~30N at around 2AM local. Created by the Author in Starry Night).

Get set for the meteoritic grand finale of summer.

Northern hemisphere summer that is. As we head into August, our gaze turns towards that “Old Faithful” of meteor showers, the Perseids. Though summer is mostly behind us now, “meteor shower season” is about to get underway in earnest.

Pronounced “Pur-SEE-ids,” this shower falls around the second week of August, just before school goes back in for most folks. This time of year also finds many the residents of the northern hemisphere out camping and away from light-polluted suburban skies.

This year also offers a special treat, as the Moon will be safely out of the sky during key observation times. The Moon reaches New phase on August 6^th at 5:51 PM EDT/ 9:51 Universal Time (UT) and will be a 32% illuminated waxing crescent around the anticipated peak for the Perseid meteors on August 12^th. And speaking of which, the Perseids are infamous for presenting a double-fisted twin peak in activity. This year, the first climax for the shower is predicted for around 13:00 UT on August 12^th, favoring Hawaii and the North American west coast, and the second peak is set to arrive 13 hours later at 02:00 UT, favoring Europe & Africa.

Nodal crossing for the Perseid stream and Earth’s orbit sits right around 18:00 to 21:00 UT on August 12^th for 2013. The shower derives its name from the constellation Perseus, and has a radiant located near Gamma Persei at right ascension 3 hours 4 minutes and a declination of +58 degrees. Atmospheric velocities for the Perseids are on the high end as meteor showers go, at 59km/sec.

Of course, like with any meteor shower, it’s worth starting to watch a few days prior to the peak date. Although meteor streams like the Perseids have been modeled and mapped over the years, there are still lots of surprises out there. Plus, starting an early vigil is insurance that you at least catch some action in the event that you’re clouded out on game day! Like we mentioned in last week’s post on the Delta Aquarids, the Perseids are already active, spanning a season from July 17^th to August 24^th.

The Zenithal Hourly Rate for the Perseids is generally between 60-100 meteors. The ZHR is the number of meteors you could expect to see during optimal conditions under dark skies with the radiant directly overhead. Rates were enhanced back in the 1990’s, and 2004 saw a ZHR of 200.

The orbit of comet Swift-Tuttle and its intersection near the Earth's orbit. (Created the author using NASA/JPL ephmeris generator). — The orbit of comet Swift-Tuttle and its intersection near the Earth’s orbit. (Created by the author using NASA/JPL ephemerides generator).

The source of the Perseids is comet 109P/Swift-Tuttle. Discovered on July 16^th-19th, 1862 by astronomers Lewis Swift & Horace Tuttle, Swift-Tuttle is on a 133.3 year orbit and last passed through the inner solar system in late 1992. This comet will once again grace our skies in early 2126 AD.

The Perseids are also sometimes referred to as the “tears of St Lawrence,” after the Catholic saint who was martyred on August 10^th, 258 AD. The Perseids have been noted by Chinese astronomers as far back as 36 AD, when it was recorded that “more than 100 meteors flew thither in the morning.” The annual nature of the shower was first described by Belgian astronomer Adolphe Quételet in 1835.

Enhanced rates for the Perseids marked the return of comet Swift-Tuttle in the 1990s. Recent years have seen rates as reported by the International Meteor Organization at a ZHR=175(2009), 91(2010), 58(2011), & a resurgence of a ZHR=122 last year.

Just what will 2013 bring? There’s one truism in meteor observing—you definitely won’t see anything if you do not get out and observe. Meteor shower observing requires no equipment, just clear skies and patience. Watch in the early hours before dawn, when the rates are highest. Meteors can occasionally be seen before midnight, but are marked by lower rates and slow, stately trains across the sky. Some suggest that best viewing is at a 45 degree angle away from the radiant, but we maintain that meteors can appear anywhere in the sky. Pair up with a friend or two and watch in opposite directions to increase your meteor-spotting chances.

We also like to keep a set of binoculars handy to examine those smoke trains left by bright fireballs that may persist seconds after streaking across the sky.

And speaking of which, there has also been some spirited discussion over the past week as to whether or not the Perseids produce more fireballs than any other shower. I certainly remember seeing several memorable fireballs from this shower over the years, although the Geminids, Leonids and Taurids can be just spectacular on active years. The stated r value of the Perseids is one of the lowest at 2.2, suggesting a statistically high percentage of fireballs.

And in the realm of the strange and the curious, here are just a few phenomena to watch/listen for on your Perseid vigil;

– Can you “hear” meteors? Science says that sounds shouldn’t carry through the tenuous atmosphere above 50 kilometres up, and yet reports of audible meteors as a hiss or crackle persist. Is this an eye-brain illusion? Researchers in 1988 actually studied this phenomenon, which is also sometimes reported during displays of aurora. If there’s anything to it, the culprit may be the localized generation of localized electrophonic noises generated by Extra/Very Low Frequency electromagnetic radiation.

– Can meteor streaks appear colored? Green is often the top reported hue.

– Can meteors appear to “corkscrew” during their trajectory, or is this an illusion?

A Perseid very near the shower radiant during the 2012 shower. (Photo by author).

Wide-field photography is definitely a viable option during meteor showers. Just remember to bring extra charged batteries, as long exposure times will drain modern DSLRs in a hurry!

And did you know: you can even “listen” to meteor pings on an FM radio or portable TV? This is a great “rain check” option!

And there’s still real science to be done in the world of meteor shower studies. The International Meteor Organization welcomes counts from volunteers… and be sure to Tweet those Perseid sightings to #Meteorwatch.

Also be sure to check out the UK Meteor Observation Network, which has just launched their live site with streaming images of meteors as they are recorded.

Good luck, clear skies, and let the late 2013 meteor shower season begin!

-And be sure to post those Perseid pics to the Flickr forum on Universe Today… we’ll be doing photo essay roundups from observers around the world!

July 30, 2013December 23, 2015 by Nancy Atkinson

Astrophotos: Views of the Delta Aquarid Meteor Shower

Delta Aquarid Meteors seen from Dayton, Ohio on July 30, 2013. Credit and copyright: John Chumack.

Did those of you in the northern hemisphere have a chance to look for the Delta Aquarid meteors? Ever-faithful astronomer and astrophotographer John Chumack captured this view overnight from his observatory near Dayton, Ohio. Can you see the two meteors in this frame?

Below is another shot from John taken on July 29 using his Meteor Video Camera Network, and he captured about half a dozen bright ones, including one meteor through the clouds.

A Delta Aquarid meteor shows up through the clouds on July 29, 2013. Credit and copyright: John Chumack.

As our own David Dickenson said in his recent “how to” post on observing the Delta Aquarids, this meteor shower “can serve as a great “dry run” for the Perseids in a few weeks. You don’t need any specialized gear, simply find a dark site, block the Moon behind a building or hill, and watch.”

And as far as photographing them, David says that technique is “similar to doing long exposures of star trails.”

Simply aim your tripod mounted DSLR camera at a section of sky and take a series of time exposures about 1-3 minutes long to reveal meteor streaks. Images of Delta Aquarids seem elusive, almost to the point of being mythical. An internet search turns up more blurry pictures of guys in ape suits purporting to be Bigfoot than Delta Aquarid images… perhaps we can document the “legendary Delta Aquarids” this year?

July 26, 2013April 26, 2016 by David Dickinson

Watch for the Delta Aquarid Meteors This Weekend

The Southern Delta Aquarid radiant, looking southeast at 2AM local from latitude 30 degrees north on the morning of July 30th. (Created by the author in Starry Night).

The meteor shower drought ends this weekend.

The northern summer hemisphere meteor season is almost upon us. In a few weeks’ time, the Perseids — the “Old Faithful” of meteor showers — will be gracing night skies worldwide.

But the Perseids have an “opening act”- a meteor shower optimized for southern hemisphere skies known as the Delta Aquarids.

This year offers a mixed bag for this shower. The Delta Aquarids are expected to peak on July 30^th and we should start seeing some action from this shower starting this weekend.

The Moon, however, also reaches Last Quarter phase the day before the expected peak of the Delta Aquarids this year on July 29^th at 1:43PM EDT/17:43 Universal Time (UT). This will diminish the visibility of all but the brightest meteors in the early morning hours of July 30^th.

A cluster of meteor shower radiants also lies nearby. The Eta Aquarids emanate from a point near the asterism known as the “Water Jar” in the constellation Aquarius around May 5^th. Another nearby but weaker shower known as the Alpha Capricornids are also currently active, with a zenithal hourly rate (ZHR) approaching the average hourly sporadic rate of 5. And speaking of which, the antihelion point, another source of sporadic meteors, is nearby in late July as well in eastern Capricornus.

The Delta Aquarids are caused by remnants of Comet 96P/Machholz colliding with Earth’s atmosphere. The short period comet was only discovered in 1986 by amateur astronomer Donald Machholz. Prior to this, the source of the Delta Aquarids was a mystery.

The Delta Aquarids have a moderate atmospheric entry velocity (for a meteor shower, that is) around an average of 41 kilometres a second. They also have one of the lowest r values of a major shower at 3.2, meaning that they produce a disproportionately higher number of fainter meteors, although occasional brighter fireballs are also associated with this shower.

Image of an early confirmed Delta Aquarid captured by the UK Fireball Network (@ on Twitter) captured by their Ash Vale North camera. — Image of an early confirmed Delta Aquarid by the UK Meteor Network (@UKMeteorNetwork on Twitter) captured by their Ash Vale North camera on July 17th, 2013. (Credit: Richard Kacerek & United Kingdom Meteor Observation Network, used with permission).

The Delta Aquarids are also one the very few showers with a southern hemisphere radiant. It’s somewhat of a mystery as to why meteor showers seem to favor the northern hemisphere. Of the 18 major annual meteor showers, only four occur below the ecliptic plane and three (the Alpha Capricornids, and the Eta and Delta Aquarids) approach the Earth from south of the equator. A statistical fluke, or just the product of the current epoch?

In fact, the Delta Aquarids have the most southern radiant of any major shower, with a radiant located just north of the bright star Fomalhaut in the constellation Piscis Austrinus near Right Ascension 339 degrees and Declination -17 degrees. Researchers have even broken this shower down into two distinct northern and southern radiants, although it’s the southern radiant that is the more active during the July season.

Together, this loose grouping of meteor shower radiants in the vicinity is known as the Aquarid-Capricornid complex. The Delta Aquarids are active from July 14^th to August 18^th, and unlike most showers, have a very broad peak. This is why you’ll see sites often quote the maximum for the shower at anywhere from July 28^th to the 31^st. In fact, you may just catch a stray Delta Aquarid while on vigil for the Perseids in a few weeks!

The shower was first identified by astronomer G.L. Tupman, who plotted 65 meteors associated with the stream in 1870. Observations of the Delta Aquarids were an off-and-on affair throughout the early 20^th century, with many charts erroneously listing them as the “Beta Piscids”. The separate northern and southern radiants weren’t even untangled until 1950. The advent of radio astronomy made more refined observations of the Delta Aquarids possible. In 1949, Canadian astronomer D.W.R. McKinley based out of Ottawa, Canada identified both streams and pinned down the 41 km per second velocity that’s still quoted for the shower today.

Further radio studies of the shower were carried out at Jodrell Bank in the early 1950’s, and the shower gave strong returns in the early 1970’s for southern hemisphere observers even with the Moon above the horizon, with ZHRs approaching 40. The best return for the Southern Delta Aquarids in recent times is listed by the International Meteor Organization as a ZHR of about 40 on the morning of July 28^th, 2009.

A study of the Delta Aquarids in 1963 by Fred Whipple and S.E. Hamid reveal striking similarities between the Delta Aquarids and the January Quadrantids & daytime Arietid stream active in June. They note that the orbital parameters of the streams were similar about 1,400 years ago, and the paths are thought to have diverged due to perturbations from the planet Jupiter.

Observing the Delta Aquarids can serve as a great “dry run” for the Perseids in a few weeks. You don’t need any specialized gear, simply find a dark site, block the Moon behind a building or hill, and watch.

Photographing meteors is similar to doing long exposures of star trails. Simply aim your tripod mounted DSLR camera at a section of sky and take a series of time exposures about 1-3 minutes long to reveal meteor streaks. Images of Delta Aquarids seem elusive, almost to the point of being mythical. An internet search turns up more blurry pictures of guys in ape suits purporting to be Bigfoot than Delta Aquarid images… perhaps we can document the “legendary Delta Aquarids” this year?

– Read more of the fascinating history of the Delta Aquarids here.

– Seen a meteor? Be sure to tweet it to #Meteorwatch.

– The IMO wants your meteor counts and observations!

July 25, 2013December 23, 2015 by Elizabeth Howell

Russian Meteorite Bits Will Be Used In Some 2014 Olympic Medals

The two main smoke trails left by the Russian meteorite as it passed over the city of Chelyabinsk. Credit: AP Photo/Chelyabinsk.ru

Going for gold in the Sochi Winter Olympics could earn athletes some out-of-this-world rocks.

Athletes who top the podium on Feb. 15, 2014 will receive special medals with pieces of the Chelyabinsk meteor that broke up over the remote Russian community on that day in 2013, according to media reports.

“We will hand out our medals to all the athletes who will win gold on that day, because both the meteorite strike and the Olympic Games are the global events,” stated Chelyabinsk Region Culture Minister Alexei Betekhtin in a Ria Novosti report.

The reported sports that will receive these medals include:

Women’s 1,000 meter and men’s 1,500 meter short track;
Men’s skeleton;
Women’s cross-country skiing relay;
Men’s K-125 ski jump;
Men’s 1,500 meter speed skating;
Women’s super giant slalom.

The 55-foot (17-meter) meteor’s airburst in February damaged buildings, causing injuries and fright among those in the region. As astronomers have been collecting fragments and calculating the orbit of the fireball, the incident put renewed attention on the need to monitor space rocks that could threaten the Earth.

Check out this Universe Today collection of videos showing what the meteor looked like.

July 23, 2013December 23, 2015 by David Dickinson

Space Debris: A Tale of Two Satellites

Artist's concept of a GOES spacecraft in orbit. (Credit: NOAA.gov).

It’s sometimes tough being a satellite in Earth orbit these days.

An interesting commentary came our way recently via NASA’s Orbital Debris Program Office’s Orbital Debris Quarterly News. The article, entitled High-Speed Particle Impacts Suspected in Two Spacecraft Anomalies, highlights a growing trend in the local space environment.

The tale begins with GOES 13 located in geostationary orbit over longitude 75° West. Launched on May 24^th, 2006 atop a Delta IV rocket, GOES 13 is an integral part of the U.S. National Oceanic and Atmospheric Administration (NOAA’s) Geostationary Operational Environmental Satellite network.

The problems began when GOES-13 began to suffer an “attitude disturbance of unknown origin” on May 22^nd of this year, causing it to drift about two degrees per hour off of its required nadir (the opposite of zenith) pointing.

The anomaly was similar to a problem encountered by the NOAA 17 spacecraft on November 20^th, 2005. At the time, the anomaly was suspected to be due to a micrometeoroid impact. The Leonid meteors, which peak right around the middle of November, were a chief suspect. However, NOAA 17 suffered a second failure 18 days later, which was later traced down to a hydrazine leak from its errant thrusters.

GOES-13 has weathered hard times before. Back in December of 2006, GOES-13’s Solar X-Ray Imager suffered damage after being struck by a solar flare shortly after initial deployment. GOES-13 also began returning degraded imagery in September 2012, forcing it into backup status for Hurricane Sandy.

GOES-13 was restored to functionality last month. Current thinking is that the satellite was struck by a micrometeorite. No major meteor showers were active at the time.

Loss of a GOES satellite would place a definite strain on our weather monitoring and Earth observing capability. Begun with the launch of GOES-1 in 1975, currently six GOES satellites are in operation, including one used to relay data for PeaceSat (GOES-7) and one used as a communications relay for the South Pole research station (GOES-3).

The GOES program cost NOAA billions in cost overruns to execute. The next GOES launch is GOES-R scheduled in 2015.

But the universe seems to love coincidences.

NEE-01 Pegaso before deployment. (Credit: Wikimedia Commons image in the Public Domain).

Less than 26 hours after the GOES 13 anomaly, Ecuador’s first satellite, NEE-01 Pegaso began to have difficulties keeping a stable attitude. The event happened shortly after passage near an old Soviet rocket booster (NORAD designation 1986-058B) which launched Kosmos 1768 on August 2^nd, 1986. The U.S. Joint Space Operations Center had warned the fledgling Ecuadorian Space Agency that conjunction was imminent, but of course, there’s not much that could’ve been done to save the tiny CubeSat.

Although the main mass passed Pegaso at a safe distance, current thinking is that the discarded booster may have left a cloud of debris in its wake. Researchers have tracked small “debris clouds” around objects it orbit before- the collision of Iridium 33 and the defunct Kosmos 2251 on February 10^th, 2009 left a ring of debris in its wake, and the Chinese anti-satellite test carried out on January 11^th, 2007 showered low-Earth orbit with debris for years to come.

The loss represents a blow to Ecuador and their first bid to become a space-faring nation. Launched less than a month prior atop a Long March 2D rocket, Pegaso was a small 10 centimetre nanosatellite equipped with solar panels and dual infrared and visible Earth imaging systems.

A translation from the Ecuadorian Space Agencies site states that;

“The NEE-01 survived the crash and remains in orbit; however it has entered uncontrolled rotation due to the event.

Due to this rotation, (the satellite) cannot point its antenna correctly and stably to the Earth station and although still transmitting and running, the signal cannot be decoded. The Ecuadorian Civilian Space Agency is working tirelessly to stabilize the NEE-01 and recover the use of their signal.

The PEGASUS aired for 7 days your signal to the world via EarthCam, millions could see the Earth seen from space in real time, many for the first time, the files in those 7 days have been published after transmission.”

Ecuador plans to launch another CubeSat, NEE 02 Krysaor later in 2013. A carrier has not yet been named.

While both events suffered by the GOES-13 and NEE-01 Pegaso satellites were unrelated, they underscore problems with space junk and space environmental hazards that are occurring with a higher frequency.

Gabbard diagram displaying a sample disintegration of a Long March 4 booster in 2000. (Credit: the NASA Orbital Debris Office).

Such is the modern hazardous environment of low Earth orbit that new satellites must face. With a growing amount of debris, impact threats are becoming more common. The International Space Station must perform frequent debris avoidance maneuvers to avoid hazards, and more than once, the crew has waited out a pass in their Soyuz escape modules should immediate evacuation become necessary. Punctures from micro-meteoroids or space junk have even been seen recently on the ISS solar panel arrays.

Plans are on the drawing board to deal with space junk, involving everything from “space nets” to lasers and even more exotic ideas. Probably the most immediate solution that can be implemented is to assure new payloads have a way to “self-terminate” via de-orbit at the end of their life span. Solar sail technologies, such as NanoSailD2 launched in 2010 have already demonstrated this capability.

Expect reentries also pick up as we approach the peak of solar cycle #24 at the end of 2013 and the beginning of 2014. Increased solar activity energizes the upper atmosphere and creates increased drag on low Earth satellites.

It’s a brave new world “up there,” and hazards, both natural and man-made, are something that space faring nations will have to come to terms with.

-Read and subscribe to the latest edition of NASA’s Orbital Debris Quarterly News for free here.