2008 09 09 The SPE Outbreak

As the sun was about to rise on September 9, 2008 an unpredicted outbreak of the September Perseid shower occurred.

Jeff, at the West Kelowna site, checked his overnight Sentinel video captures and quickly noted an unusual cluster of fireballs. Below is a composite image of of the outbreak.

Brower notified Dr. Peter Jenniskens of the large number of fireballs via e-mail. Jenniskens then sent inquiries to other observers to confirm the outbreak. Almost simultaneously reports of the outbreak started coming in on various meteor forums . As soon as Jenniskens received supporting information he issued a telegram, CBET 1501, as shown below.

CBET 1501 SPE 2008

 

Fall 2016 Meteor Showers

Meteor Showers in Oct, Nov, Dec 2016.

**The Geminids are the best at 120 meteors per hour, are on 14 Dec.  *The Orionids (21 Oct) and the Leonids (17 Nov) both at 15 meteors per hour are middling.  The Northern Taurids on 12 Nov at 5 meteors per hour aren’t as frequent but they produce many bright fireballs, and flashes on the Moon.  However, the bright Moon will spoil much of the meteor showers this year.  Meteor velocities can range from about 11 km/s (very slow) to 72 km/s (very fast). 40 km/s is roughly medium speed.  (That’s still pretty fast. For comparison, the International space station orbits at 8km/s, and goes around the Earth in 90 minutes.)  These meteors travel across the sky very swiftly, with “trains”.  Look for a series of small explosions in the meteor trail as the rock breaks up. Some leave a luminous train of particles that last for a few seconds or even a minute. Colours can be yellow to brilliant green. You may hear a delayed supersonic rumble (5 minutes later) if a fireball comes close overhead and a chirp of descending pitch on a shortwave radio, from the meteors ion plasma.

 *Fri 21 Oct: The ORIONIDs: Active: Oct 02–Nov 07 with maximum on Friday Oct 21;  The zenith hourly rate (ZHR) is  15 meteors/hr; with a fast speed of 66 km/s, the remnants of Comet Halley.  This year is likely a typical shower at 15 meteors per hour.   This can vary from year to year, with a 12 year cycle of strong and weak peaks ranging from 14 to 31 meteors per hour; and another factor which can produce outbursts of 70 meteors/hr.  The Moon will rise around midnight at its last quarter (65%-illuminated) which bright glow will drown out the fainter meteors.  The meteors should radiate out from the North part of Orion the Hunter, by his club, on the Eastern horizon.  Since the Moon is located quite close to the radiant at this time it will spoil all optical observations.

 These meteors consist of falling ice pellets, dust and sand debris encountered as the Earth crosses the orbit of Halley’s Comet, coming in fast at 66 km per second. This debris moves parallel to itself along the orbit of the comet, thus from our Earth perspective it looks like they radiate out from a single point, the “radiant”. The Orionids all appear to radiate out from Orion, the streaks looking like huge bicycle spokes with the centre hub at Orion’s shoulder.  They are visible coming from the Eastern horizon when Orion rises after midnight towards 1 to 6am. The half of the meteors that go below the horizon won’t be seen. You should be out of town where it’s dark to see them best. Don’t look towards the East, these trails will look short due to foreshortening.  Instead look 90 degrees away, either straight overhead, or to the North, away from the Moon’s bright light.

 Sat 12 Nov: The Northern TAURIDs: (Active: Oct 20 to Dec 10, max on 12 Nov).  The zenith hourly rate (ZHR) is  just 5 meteors/hour; velocity a slow 29km/s. The Earth passes through a debris stream left by Comet Encke, source of the Taurid Meteor Shower.  Taurid meteors tend to be larger than average: they are bright, with many fireballs. They also penetrate deeper into the Earth’s atmosphere than other meteors. For example, Orionids typically burn up at altitudes of 93 km, but the Taurids make it down to 68 km. Some get even lower — meteor cameras have tracked 1-inch Northern Taurid meteors down to 58 km.

 

Moon Impacts: Because the Taurid Meteors can be 1 inch bullets of ice moving at 29 km/s (which is a hypersonic mach 88), they produce bright flashes of light when they strike the Moon. Taurid lunar impacts are visible with the college’s 10″ or 11” Schmidt-Cassegrain telescopes as small flickers of light, in dark regions.  However, since the moon is 94% illuminated on Nov 12, there’s not much dark area to look into.  But sometimes you can see brighter flashes in the illuminated area as well.  Some telescopes are fitted with video cameras and count how many meteors hit the Moon overall.  One impact imaged on Sep 2013 was so hot it glowed white hot for 8 seconds–it was estimated to be a 40kg rock.

 *Thu 17 Nov: The LEONIDs Active: Nov 06–Nov 30 Nov 17; Maximum: Thu Nov 17; ZHR = 15 meteors/hr; V = 71 km/s.  These arrive just three days after the full Moon, which will make it hard to see them.  There are a lot of fast green meteors in the Leonids.

 Mon 28 Nov: The November Orionids.  Active: November 14–December 6; Maximum: Monday Nov 28;  ZHR = 3 meteors/hr; V = 44 km/s

**Wed 14 Dec: The GEMINIDS; active Dec 04–Dec 17; Maximum: Dec 14; ZHR = 120 meteors/hr; V= 35 km/s.

The best and most reliable meteor shower of the year are the Geminids at 120 meteors per hour on Wednesday, December 14.  Except we have the Full Moon on the same night to spoil them.  The Geminid meteors are debris from an extinct comet (called 3200 Phaethon) coming in at 35 km/second.  (That’s a medium speed for a meteor.  Other meteor shower velocities range from 11 to 72 km/s.) The Geminids come in various colours–65% being white, 26% yellow, and the remaining 9% blue, red and green.  The meteors are the sand, dust and gravel remains of an Apollo asteroid (3200 Phaethon), coming in at medium speeds of 35km/second.    

Colourful meteor here taken by Robert Ede in Invermere, against the Milky Way to the South.  Note the colour in the trail starts green and turns red.  

 Fireball Colours: Green can be caused by copper or magnesium metal burning. Other colours seen are yellow, orange and red.  Iron burns yellow (eg. steel wool), silicates burn red and sodium burns orange.

 Ionization trails: Sometimes the wakes behind them can be ionized oxygen emitting green light. That occurs at higher altitudes where the air pressure is low. The higher collision energies make oxygen produce a greenish glow, nitrogen emits blue and red, at the lower energies a dim red. Just like the colours in the Northern Lights. So, fast meteors would have more energy and produce more greens and blues, slow meteors would have lower energy and produce reds.

 Which direction is best to look? Where it’s darkest. As you can see in these composite photos from last year, the fireballs scatter all over the sky, radiating out from Gemini to the East. But when you watch the area around Gemini, the streaks there are shorter and slower moving. These fisheye photos show the whole sky as a circle: North is up, South down, East to the left, and West to right.

 

All the brighter Geminid Meteors during the night of 14 Dec 2014.   The photos were taken with the College of the Rockies meteor cam in Cranbrook, BC. 

 

It is thought the Geminids originated from an asteroid named 3200 Phaethon, discovered in 1983.  It may be a small 5km fragment from the 544km main belt asteroid Pallas

 

 

2008 02 19 PNW Bolide

On February 19, 2008 at 13:30 UT, a large fireball entered the earth’s upper atmosphere. Visual reports of the bolide started streaming in at police stations and television stations. A regional airline pilot filed a report of a possible aircraft going down over western Washington.

At 13:30:59 UT the West Kelowna Sentinel all-sky camera caught was triggered by a extremely bright bolide. The video showed the bolide moving slowly downward towards my southeastern horizon. It disappeared behind the mountains across the Okanagan Lake. Despite being below my horizon behind the mountain range the sky pulsed with light as the bolide went through several terminal bursts as can be seen by the total amplitude light curve produced by the Sentinel camera:

 

A look at the total number of pixels above the triggering threshold shows most of the light was released during it’s terminal flares.

Total Pixels graph

The graphs as well as the movie was sent to Dr. Alan Hildebrand, Coordinator of the Canadian Fireball Reporting Centre, University of Calgary.

 

2002 11 19 Leonids Outbreak

Hiroshi Ogawa, head of the International Project for Radio Meteor Observation,  asked radio detection stations from around the world to observe the Leonids during the period of November 1 to November 25, 2002.

Note: Brower was located in Loveland, Colorado at the time of the study and not in West Kelowna.

The following graph shows three stations located in Slovenia, USA, and Japan. The three stations data help trace  the overall activity of the 2002 Leonids.  Notice how as the radian lowered in the sky in Slovenia the radiant was rising for Colorado. Similarly, as the radiant dipped to the west of Colorado it was climbing higher in the sky in Japan, thus giving a continuous view of the overall stream activity over time.

FS Radio results Leo 2002

One of the most rewarding part of the 2002 Leonid study was the recording of a predicted filament  of the comet’s ejecta by Yrjöllä and Brower.

In chapter 14 of Jennniskens book, Meteor Showers and their Parents (Jenniskens 2006:201-215) gives a detail discussion of the filament and why it is important. He states:

Jupiter’s past perturbations may have responsible for the sudden onset of the component in 1994…
I expected the dust component would remain visible post perihelion for at least slightly less than one orbit of Jupiter (<12 yr), thus until 2004 or 2005.

I saw this validated in 2002, when the Filament component was detected for the first time after the perihelion passage of the comet, underlying two very narrow Leonid storm profiles (Fig. 14.41) The observed shift in the peak time and constant width over the years 1994 to 2002 (Table 4) confirms that this component moves about the earth’s path much like individual dust trails in reflection to the ever changing gravitational field of the planets (shaded area in Fig 14.15). Again, more or less following the sun’s reflex motion. (Ibid:214-215)

(Place Fig 14-41 Yrjöllä and Brower here)

More to come…

Jenniskens, P. 2006. Meteor Showers and their Parents, Cambridge University Press, Cambridge, U.K.

Perseid Meteor Shower Thursday 11 Aug 2016

The college meteor camera is already seeing more bright meteors zipping overhead. The Perseid meteor shower started July 17, ends Aug 24 but peaks on Thursday night, August 11 and Friday morning Aug 12. If it’s cloudy Thursday, note that Wednesday night and Friday night will also be very active.

This year the Earth will cross the centre of the comet debris; so we should get the full show. We should also get three additional early peaks: Jupiter’s gravity has shifted some debris; and we’ll see debris from the 1862 and 1479 comet ejection trails to hit this year. Peak estimates (by Esko Lyytinen and Mikhail Maslov) are 150 to 160 meteors per hour, about three per minute.

There are four peaks in two waves; we’ll miss the first wave since it hits Thursday in daylight; and the last wave which hits in Friday’s morning light. But the whole night should be pretty constant at 100 meteors/hour. Best seeing times in the East Kootenays would be after midnight once the Moon sets (low in Scorpius) and the skies darken; continuing until dawn at 5am. We’ll miss the last wave at 7am. But these peak times are estimates, we can hope they arrive during darkness instead.

  (Mountain Daylight Savings Time-- minus 1 hr for Pacific) 1.  Thurs Aug 11 at 4:34pm [1862 comet trail] 2.  Aug 11 at 5:24pm [1479 comet trail] 3.  Aug 11 from 6 to 10pm [Jupiter shifts] 4.  Fri Aug 12 from 7 to 9am [Centre of comet orbit].  

It takes the Earth a week to pass through all the ice and dust from comet Swift-Tuttle. The shower will gradually taper off and end by Aug 24. The meteors are travelling at a speed of 59 km/s when they enter the Earth’s atmosphere. Their trails will all point to Perseus (if it’s a Perseid). The closer they are, the smaller their trail: and the further away, the longer the trail. Look for their colours—at high speed they ionize the air to a green; then that fades to yellow, orange, red as it slows down. If they disrupt and flare, you may see green/bluish wide streaks that glow afterward for a second or two (mainly it’s water ice, but there may be metals present like copper or cobalt).

Allsky Cam Meteor Images Aug 11-12
Allsky Cam Meteor Images Aug 11-12

Where to look? The composite photo above shows the entire sky, and all the meteors that fell on 11 and 12 Aug 2015 over Cranbrook; taken by our college meteor camera. Perseus is the constellation to the North East (middle left side of the photo). Normally there are fewer meteors seen straight overhead, since there is less volume of atmosphere overhead. There are slightly more meteors seen high to the West around Hercules and above the handle of the big dipper; since the meteor trails are longer there, and the meteors skim lower in a greater volume of atmosphere. That’s where I aim my cameras. (Or where it’s darkest, away from the Moon or city streetlight glow).

Allsky Captures Stacked for 13 Aug 2015
Allsky Captures Stacked for 13 Aug 2015

Some of the meteors seen will be from the k-Cygnids running from August 6–19. These peak on August 18 at 3 meteors per hour. They show a number of slow falling fireballs moving at 25km/second.

Small Fireball from Cygnus
Small k-Cygnid Fireball Crossing Cygnus

This photo shows a k-Cygnid meteor crossing through Cygnus the Swan as seen during the last Perseid shower of 2015 (it’s tail is short and it points from Cygnus). Photo taken with a Nikon D100, Tamron 28mm f/2.5 lens, 30 second exposure. I outlined Cygnus in yellow against the Milky Way. The bright star Deneb is the tail at top, and Albireo is the beak at bottom. Photo credit: Rick Nowell.

Starmap of Northeast Sky with Perseus for 13Aug
Starmap of Northeast Sky with Perseus for 13Aug

While you’re out stargazing, here is a starmap showing the Perseus region of the sky, looking Northeast late after midnight in August. The Milky Way band (grey in the map) runs through Perseus; who is the Greek hero coming to rescue Andromeda (daughter of Cassiopeia) who is chained to the rocks. Look below the W of Cassiopeia (the Queen of Ethiopia). You should also see the great square of Pegasus, the winged horse to the right. If you have good eyes (or binoculars), you can spot the fuzzy cloud of the Andromeda Galaxy (M31 in the Map) just above Andromeda’s stick-figure knee. (Andromeda’s head is one corner of the square of Pegasus.) The big dipper, little dipper and Polaris are easy to locate to the left. (Starmap generated by Skyglobe software).

Note: to zoom in a picture or map and see the lines, right-click and open in new tab.

Preparation for calibrating a Sentinel Camera

Steps to take prior to calibrating a Sentinel Camera

Flesh out – PLACEHOLDER ONLY!

Put the procedure here.

  1. Make long exposure after each capture… TIF format
  2. Use GIMP, Paint, PhotoShop or other image processing program and push the brightness and contrast
  3. After photo brings out the hidden starts run a planetarium program. Looking south, elv 90, fov 180.
  4. Match the stars noting pixel x/y on photo and az/el on the planetarium.
  5. run python program calpos.py This produces a personalized correction file that will be used for triangulation. (See Ken’s pdf on the process)