Dec 13/14 Geminids Recap

Last night marked the probable peak of the 2014 Geminids. Here in Tucson, we had rain during the day (0.27″) and it was looking iffy as to whether the night would remain clear of clouds and fog. I spent 1h 15m outside between 10:17 and 11:33 pm local time. Though it was very muggy and it sounded like it was still rainy as condensation dripped off the house, the night turned out to be a good one for meteor watching. I was consistently seeing 12-14 Geminids every 15 minutes so just under 1 per minute (with a limiting magnitude of ~6.1).

My camera system had an even better night as it detected 179 meteors of which 139 were Geminids over the course of the night. That is a new record for my meteor camera system having beaten the peak night of the 2010 Geminids by 20 meteors. I will try to get a video from my camera online shortly.

Geminid activity rapidly falls off after the peak. Observers may still be able to see a good number of Geminids tonight though rates will be 1/4 to 1/2 what they were last night.

The International Meteor Organization (IMO) maintains a “live” graph showing the rate of the Geminids as reported by visual observers around the world.

Obs Date(UT)     Time    TOT SPO ANT GEM HYD COM Others
VIS 2014-12-14  01h 16m   71  6   -   65  -   -     -   LM=6.0-6.1
SAL 2014-12-14  12h 41m  179  21  7  139  2   2     8

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
GEM - Geminids
HYD - Sigma Hydrids
COM - Comae Berenicids
Others - other minor showers

Here Comes the Geminids!

Tonight is one of the best nights of the year to see a meteor as the Geminid meteor shower is predicted to reach its 2014 peak. The Geminids are one of two annual showers (the other being August’s Perseids) that are almost guaranteed to produce high rates of meteors (at least one every few minutes or better).

The International Meteor Organization (IMO) maintains a “live” graph showing the rate of the Geminids as reported by visual observers around the world.

How To See Them

This year the Geminids will be near peak intensity on Saturday night/Sunday morning, December 13/14. From a dark, moon-less sky, the Geminids have consistently produced peak rates of ~100 meteors per hour. According to the IMO, the Geminids reached ZHR rates of 134 per hour in 2013, 109 in 2012, 198 in 2011, 127 in 2010, 120 in 2009, 139 in 2008, 122 in 2007 and 115 in 2006. Note, these rates assume ideal observing circumstances that are rarely achieved. Dark sky observers may see rates that approach the ZHR values. Most of us observing under light polluted skies will see lower rates (perhaps much lower for city dwellers or observers watching before 10pm).

Unlike most showers that can only be observed in the early hours of the morning, the Geminids radiant rises as early as 7 pm and a good number of meteors can be seen by 10 pm. The radiant is nearly overhead at 2 am and it still well placed for the rest of the night. This year the Last Quarter Moon (located close to a brilliant Jupiter) will hinder Geminid watching after midnight. The shower can still be observed after Moonrise though fainter meteors will be washed out. It helps to keep the Moon out of your line of sight.

As the name implies, the Geminids appear to radiate from a point in the constellation of Gemini. More specifically from a point just to the north of the bright star Castor, the northern star in the Castor-Pollux pair. During the evening Geminids will be coming out of the northeast. By the middle of the night the radiant will be close to overhead and meteors will be raining down on all sides.

In general it is best not to look directly at the radiant. Meteors are easier to see by looking 30 or more degrees from the radiant (for reference 10 degrees is the width of your hand at arms length). The key is to look up and regardless of where you look you should see quite a few Geminids.

2014_Geminids

The night sky for December 13 at 11:00pm local time over Tucson. The Geminid radiant is shown as a yellow circle with Geminid meteors radiating away from it. Chart produced with Stellarium.

.

Sky brightness matters when it comes to seeing most meteors and the Geminids are no exception. As always, the darker the sky the better. If you are located in a place with pitch black skies (mountaintops, middle of the desert, national parks) rates can be as high as ~100 per hour. In rural areas near small towns rates will be a bit lower and probably in the 80-90 per hour range. In the suburbs rates will vary depending on how close to a major city you are but you should expect rates of 20-50 per hour. In a major city rates will be very low though 2-10 per hour should be seen.

To increase your chance of seeing the Geminids find a spot with a clear view of the sky. Any obstructions (trees, buildings, etc.) can block some of the meteors. Also find a spot where lights (streetlights, security lights, etc.) aren’t shining in your eyes. This will allow your eyes to dark adapt and you will be able to see fainter, and more, meteors. The most important thing to remember is to get comfortable when observing. A lawn chair is perfect for reclining back and taking in the sky. Remember that it is cold this time of the year in the Northern Hemisphere so bundle up. It does not take much time, especially when relatively inactive, to start freezing.

Where They Come From

The Geminids were created by an enigmatic object named (3200) Phaethon. For starters Phaethon is an asteroid and only displayed what might be considered cometary activity for a few days in 2009. But meteor showers are created by comets and nearly all comets have orbits that carry them at least as far from the Sun as the orbit of Jupiter. Yet Phaethon only travels out to a distance of 2.4 AU, roughly half the distance to Jupiter’s orbit. Based on its orbit it is hard to call Phaethon anything but an asteroid.

Phaethon2014

Image of Geminid parent body (3200) Phaethon by Jean-Baptiste Kikwaya on 2014 November 27 with the Vatican Observatory VATT 1.8-m.

So what is Phaethon?

1) Phaethon could be a comet whose original orbit evolved into its current one after many millennia of close approaches with the inner planets. The probability of this happening is extremely low. Some models of the formation of the Geminids require the shower particles to be released over many centuries to millennia which is consistent with the behavior of a comet. Then again…

2) Phaethon may be a Main-Belt comet. Main-Belt comets are objects that originate in the outer Asteroid, or Main, Belt. Since they contain a sizable fraction of volatile ices, they can occasionally exhibit cometary activity. Four of these objects have been observed to display cometary activity in the Main Belt. Since they start on asteroid orbits, it is not too difficult for one of them to find itself on an orbit similar to Phaethon. Or behind door #3…

3) Phaethon is an asteroid that broke up in the past. There is evidence to suggest that Phaethon is just the largest piece of a ancient break-up. In fact, two additional asteroids that may once have been a part of Phaethon have been found, (155140) 2005 UD and 1999 YC. According to Peter Jennisken’s book “Meteor Showers and Their Parent Comets”, the Geminids can be explained by the break-up of Phaethon just after perihelion many orbits ago. Since Phaethon gets to within 0.14 AU (14% of the Earth-Sun distance), perhaps it split from the stress of intense solar heating. BTW, this scenario does not rule out Phaethon as a ice-rich Main-Belt comet.

The recent discovery of additional asteroids related to Phaethon points to scenario 3 as the most likely origin of the Geminids. If true, the Geminids were not the result of long-term cometary activity like most meteor showers but were created in a discrete event or events when Phaethon split or shed smaller pieces. The Daytime Sextentids and perhaps the very minor Canis Minorids were created by even older break-up events.

Though Phaethon has behaved like an asteroid since its discovery in 1983 it has been observed to ‘burp’. Near its perihelion, the asteroid is sometimes visible in near-Sun images taken with the STEREO spacecraft and occasionally appears to elongate as if it had a short tail and brighten. Analysis by David Jewitt and Jing Li (UCLA) found that Phaethon did release some surface particles. Due to intense heating (perihelion is 0.14 AU from the Sun or 7 times closer than the Earth is) some of the rocks on the surface may have fractured producing a cloud of dust which was knocked off the surface by solar radiation pressure. In effect, it is a rock comet. Still this event was very short-lived and produced a minimal amount of debris. So these type of events should not have been large enough to create the Geminids by themselves.

I penned a guest post on Phaethon for Dr. Dante Lauretta (PI of NASA’s OSIRIS-REx asteroid sample return mission) back in 2013. You can read it here.

Whether Phaeton is a traditional comet, a volatile-rich asteroid, an asteroid that split into pieces, or a ‘rock comet’, the result is going to be one of the best astronomical shows of the year. So go out and enjoy the show!

August 11-20 Meteors

The Perseids peaked on the night of August 13 UT. Though the monsoon was still cranking and clouds were aplenty, 36 PER were detectedby the SALSA3 camera system.

Visual reports to the IMO show a peak ZHR of ~68. This is the true rate of the shower after correcting for the effects of the Moon-lit sky and the height of the radiant. Since 2007 the peak ZHR of the PERZ have ranged from 58 to as high as 180. 2014’s ZHR of 68 is the 2nd lowest of the past 8 years.

per2014overview

ZHR Live chart for the 2014 Persieds. Credit: International Meteor Organization.

Obs Date(UT)    Time   TOT SPO ANT CAP PER SDA ERI ATR KCG BAR MPR UCE
SAL 2014-08-20 07h 07m  25  17  3   -   3   1   -   1   0   -   -   0
SAL 2014-08-19 00h 36m  2   1   1   -   0   0   -   0   0   -   -   0
SAL 2014-08-18 03h 23m  4   2   1   -   0   0   0   0   1   -   -   0
SAL 2014-08-17 02h 22m  7   5   1   -   1   0   0   0   0   -   0   0
SAL 2014-08-16 04h 43m  16  8   1   -   4   0   0   1   1   -   1   -
SAL 2014-08-15 01h 12m  4   1   0   -   2   0   0   0   1   -   0   -
SAL 2014-08-14 07h 27m  42  9   4   -   20  0   0   1   4   -   3   -
SAL 2014-08-13 03h 10m  40  1   0   -   36  0   2   0   0   -   1   -
SAL 2014-08-12 02h 18m  22  2   1   0   16  1   0   1   0   1   0   -
SAL 2014-08-11 02h 12m  16  3   0   1   8   0   0   1   1   1   1   -

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
CAP - Alpha Capricornids
PER - Perseids
SDA - Southern Delta Aquariids
ERI - Eta Eridanids
ATR - Alpha Triangulids
KCG - Kappa Cygnids
BAR - Beta Arietids
MPR - Mu Perseids
UCE - Upsilon Cetids

August 9-10 Meteors

The past two nights have been a mix of meteor showers and rain showers. Luckily the sky has been clear enough, long enough to still catch one or two dozen meteors per night. Even with the patchy coverage, you can see that the Perseids are the most active shower. Visual observers for the IMO are reporting ZHRs between 20-35. Rates should reach between 60-120 by the middle of the week. Over the past few years the Perseids have peaked at ZHRs of 109 (2013), 90-120 (2012), 58 (2011), 91 (2010), 140-180 (2009), 116 (2008), and 93 (2007). We’ll have to wait and watch to see what this year’s Perseids have in store though the nearly Full Moon will hamper the number of Perseids that can be seen.

The Perseids (PER) will peak on Wednesday morning August 13 UT. Bob Lunsford as written an excellent guide on how to observe this year’s Perseids for the American Meteor Society here.

 

Obs Date(UT)    Time   TOT SPO ANT CAP PAU PER SDA SIA ERI ATR KCG BAR MPR
SAL 2014-08-10 04h 55m  23  7   0   2   1   9   0   -   2   1   1   0   0
SAL 2014-08-09 03h 15m  13  4   1   1   0   4   1   0   0   0   1   1   0

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
CAP - Alpha Capricornids
PAU - Piscis Austrinids
PER - Perseids
SDA - Southern Delta Aquariids
SIA - Southern Iota Aquariids
ERI - Eta Eridanids
ATR - Alpha Triangulids
KCG - Kappa Cygnids
BAR - Beta Arietids
MPR - Mu Perseids

August 8 meteors

Yet another good night of meteor watching by the SALSA3 video system. Meteor totals increased by 2 to 47 over the previous night. Though the number of Southern Delta Aquariids (SDA) dropped from 7 to 2, the Perseids (PER) continue their steady climb to next week’s peak as their nightly number increased from 17 to 25.

The system also started monitoring a new meteor shower, the Mu Perseids (MPR). Though the MPR are located close to the radiant of the major PER shower (and it is possible that these are PER that were misidentified by the MetRec software), they have different orbits from the PER. The shower was only recognized in 2012 by Japanese video meteor watchers.

The best meteor of the night was this Perseid from 10:30 UT.

055119

Obs Date(UT)    Time   TOT SPO ANT CAP PAU PER SDA SIA ERI ATR KCG BAR MPR
SAL 2014-08-08 08h 54m  47  14  1   0   1   25  2   0   0   0   1   1   2

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
CAP - Alpha Capricornids
PAU - Piscis Austrinids
PER - Perseids
SDA - Southern Delta Aquariids
SIA - Southern Iota Aquariids
ERI - Eta Eridanids
ATR - Alpha Triangulids
KCG - Kappa Cygnids
BAR - Beta Arietids
MPR - Mu Perseids

Aug 6 Meteors

That’s more like it. With the software timing issue fixed (it was shutting down my system a good 2-3 hours prior to dawn), my nightly total jumped from ~20 to 45 meteors. The higher number really highlights how the last 2-3 hours of the night is best for meteor watching.

Two showers account for 24 of the 45 meteors. The Southern Delta Aquariids peaked a week ago but are still producing a good number of meteors. The Perseids are the main shower visible right now. They are building towards a peak on the night of August 12/13. According to visual reports submitted to the International Meteor Organization (IMO), the Perseids are already producing ZHR rates of ~20 per hour. [Note, that ZHRs are idealized rates for perfect observing circumstances. Most observers will see lower rates in the 5-10 per hour range.] On the night of the peak, ZHRs may reach ~60-150 per hour though a very bright near Full Moon will greatly decrease the rates actually seen.

Obs Date(UT)    Time   TOT SPO ANT CAP PAU PER SDA SIA ERI ATR KCG BAR
SAL 2014-08-07 09h 06m  45  12  2   1   0   17  7   2   2   1   1   0
                  also no PPS or SIA were seen over the 3 nights

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
CAP - Alpha Capricornids
PAU - Piscis Austrinids
PER - Perseids
SDA - Southern Delta Aquariids
SIA - Southern Iota Aquariids
ERI - Eta Eridanids
ATR - Alpha Triangulids
KCG - Kappa Cygnids
BAR - Beta Arietids

July 31 – Aug 5 Meteors

The monsoon wiped out the first three night of August. Happily, these clouds did bring a bit of rain.

The nights of August 4-6 UT were very disappointing for my meteor detection network. Early August is a busy time for meteor watching with the Perseids (PER) ramping up and the various Aquarius (SDA,SIA)/Capricornus (CAP) showers still producing. I fully expected to be detecting many 10s of meteors per night rather than the lowly 20-21. At that rate, I wasn’t detecting any more meteors than back in late June.

Turns out it was a bit of an upgrade issue. The night of July 31 saw me using the newest version of MetRec (the automatic meteor detection software I use). At first I thought my camera was on its last legs as these cameras are known to loss sensitivity with time. As it turns out, one of the configuration files for MetRec got confused resulting in the software shutting down 2-3 hours before dawn. Since the last hours of the night see the highest meteor rates, it really put a dent in detections. As of August 7 UT, the problem has been fixed.

Obs Date(UT)    Time   TOT SPO ANT CAP JPE PAU PER SDA ERI ATR BCA KCG BAR
SAL 2014-08-06 06h 20m  20  9   2   0   -   1   3   3   0   1   -   0   1
SAL 2014-08-05 06h 27m  20  8   2   2   0   0   1   2   0   2   1   2   -
SAL 2014-08-04 06h 06m  21  10  0   1   1   1   2   3   0   0   0   -   -
SAL 2014-08-03 00h 00m             Clouds/rain all night
SAL 2014-08-02 00h 00m             Clouds/rain all night
SAL 2014-08-01 00h 00m             Clouds/rain all night
SAL 2014-07-31 03h 35m  10  5   0   0   0   0   3   2   0   0   0   -   -
                  also no PPS or SIA were seen over the 3 nights

SAL - SALSA3 camera in Tucson (Carl Hergenrother)
VIS - Visual observations from Tucson (Carl Hergenrother)
Time - Total amount of time each camera looked for meteors 
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
PPS - Phi Piscids
CAP - Alpha Capricornids
JPE - July Pegasids
PAU - Piscis Austrinids
PER - Perseids
SDA - Southern Delta Aquariids
SIA - Southern Iota Aquariids
ERI - Eta Eridanids
ATR - Alpha Triangulids
BCA - Beta Cassiopeiids
KCG - Kappa Cygnids
BAR - Beta Arietids
Follow

Get every new post delivered to your Inbox.

Join 106 other followers