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Mission statement - CAMS is an automated video surveillance of the night sky to validate the IAU Working List of Meteor Showers. [Contact]

eye Report fireball sightings here.

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View CAMS data

CAMS Meteoroid Orbit Database v2.0
[CAMS California (73 Mb)]
[CAMS BeNeLux]
[Documentation]

Meteorite falls:
White Mountains (2016-06-02)
Creston fall (2015-10-24)
Chelyabinsk fall (2013-02-15)
Novato fall (2012-10-17)
Sutter's Mill fall (2012-04-22)

Report possible meteorite finds in the CAMS networks: Petrus.M.Jenniskens@nasa.gov

Contacts:

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Dr. Peter Jenniskens,
SETI Institute, Principal Investigator [email];
[Career pages]

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Peter S. Gural,
Meteor detection algoritms;
POC CAMS Mid-Atlantic
[email]

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Dave Samuels,
Network operations
[email]

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Steve Rau,
Network installation/upgrades
[email]

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Jim Albers,
CAMS station Sunnyvale

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Rick Morales,
CAMS Fremont Peak

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Bryant Grigsby,
CAMS Lick Observatory

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Andy Howell,
Coordination of CAMS Florida

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Nick Moskovitz,
Coordination of LO-CAMS

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Carl Johannink,
Coordination CAMS BeNeLux

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Prof. Jack Baggaley,
Coordination CAMS New Zealand

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Mohammad Odeh,
Coordination UACN

CAMS California:
CAMS Florida:
CAMS Mid Atlantic:
LO-CAMS Arizona:


News blog:

2017, November 22 - Peter Jenniskens reports that the five computers at Fremont Peak Observatory were replaced by a single PC last Sunday, in an ongoing effort to automate the CAMS data reduction pipeline. After several cloudy nights, last night was clear and the first set of observations was transmitted and posted autonomously on the CAMS near-real time reporting site this afternoon. Three meteors were identified as alpha Monocerotids, from an unknown potentially hazardous long-period comet.

Leonid fireball

2017, November 19 - Many bright Leonids were detected in the CAMS network on November 19. The picture above is by Klaas Jobse. [More here]

Four fireballs

2017, November 15 - Nick Moskovitz reports that a bright fireball was detected by the LO-CAMS network just north of Phoenix. The American Meteor Society received over 1320 fireball reports from about 4 different events that occurred over the US, France, and Germany within ten hours. Two events were linked to the Taurid meteor shower, but initial data reduction of the CAMS trajectories shows that the Arizona fireball had a radiant near the pole. The initial entry speed was a high 26 km/s. No radar signature from falling stones was detected, but some meteorites may have fallen in the White Mountains. [More here]

2017-056B Progress
Re-entry of a Progress rocket body (UACN3 data).

2017, October 14 - Mohammad Odeh reports that the United Arab Emirates Astronomical Camera Network (UACN) is back online, in part thanks to a generous donation from the ISP provider Etisalat. Two of the three stations are back in operation. During the third night in action, both stations UACN1 and UACN3 captured the widely reported 2017-056B Progress rocket body re-entry over the Arab Peninsula at 19:29:34 local time (UTC +4h) on October 16. The network also made a nice detection of the compact October Ursae Majorids shower that night. Nightly reports of meteor shower activity from the UACN are here. Because of its location, UACN results are available shortly afer 8 UTC, the first data of last nights meteor shower radiants to be reported each day.

OCU

2017, October 14 - A nice return of the October Ursae Marjorids (shower 333) was observed by the UANC, LOCAMS and California networks October 14-16. Go here and select dates around 2017-10-15.

2017, October 6 - A predicted outburst of October Camelopardalids was detected by the CAMS BeNeLux network.

BeNeLux coverage

2017, October 3 - Paul Roggemans reports that the CAMS BeNeLux network has grown to 88 operational cameras. At Grapfontaine, two Watec cameras were installed at the Observatoire Centre Ardennes . The cameras cover the same area over Belgium that is covered by the BRAMS radio-MS project by BIRA. A number of other stations were expanded, including Ermelo, where Koen Miskote added 2 cameras for a total of four, aimed at a common survey area to the north. At Ooltgenplaat, Piet Neels added four cameras for a total of eight. At nearby Oostkapelle, Klaas Jobse also expanded to eight cameras. In Mechelen, Luc Gobin added two cameras and Paul Roggemans added one camera so that 10 cameras are now operating at this site. In Terschelling, in the northern part of the Netherlands, Piet Neels and Robert Haas added 4 new cameras. In Texel, Robert Haas added 3 new cameras. And in Zoersel, Bart Dessoy expanded to 5 cameras. The new stations are run by a new version of AutoCAMS developed by Steve Rau.

2017, September 28 - Peter Jenniskens added a new capability to the CAMS data sphere that enables a comparisson with data collected in previous years for that date. Click on "Past Data" and a new window tab will appear, click on the tabs at the top of the browser window to flip from present to past data and back to spot meteor outbursts.

2017, September 21 - Marcelo de Cicco presented the FDL effort in a talk at the International Meteor Conference in Petnica, Serbia. Pete Gural spoke about the new improvements to the trajectory solver code.

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2017, September 8 - A new web portal for CAMS data visualization has come online. It is now possible to see last night's meteor detections by the LOCAMS and Florida networks and the most recently reduced data from the BeNeLux network by Martin Breukers and Carl Johannink. Just go to http://cams.seti.org/FDL/ and choose the date from the "Pick a date" window. Data from the other CAMS networks will gradually come online in the coming months.

This new web tool is part of an effort by Frontier Development Lab 2017, a NASA research accelerator program at the SETI Institute, led by James Parr and Bill Diamond and supported by NVidia and IBM amongst others, that set out to use artificial intelligence techniques to automate the CAMS data reduction pipeline.

Over the summer, CAMS software tools have been updated by Pete Gural to run in batch mode. Python scripts designed by Jack Collison, Peter Jenniskens, and Siddha Ganju collect the submitted files, run the CAMS software, and compare the calculated orbit with a meteor shower template file based on showers assigned by Jenniskens. The new web tool designed by Jenniskens, Ganju and Leo Silverberg displays each shower radiant in sun-centered ecliptic coordinates, with a color assigned proportional to the entry speed. By hovering the cursor over a colored meteor radiant, one can see the IAU shower number. Clicking brings up a new window that shows the 2010-2016 CAMS data for that shower displayed in the planetarium program by Ian Webster. That makes the new web tool a portal to the minor showers in Webster's visualization program.

At the moment, the reduction of CAMS data from California and New Zealand is still very slow due to numerous false detections (clouds, birds, planes...). During the summer, Susana Zoghbi, Antonio Ordonez, Marcelo de Cicco, and Pete Gural developed machine learning and deep-learning tools to discriminate meteors from other detections. Gural will use this to improve future versions of the Confirmation and Coincidence programs. Further improvements are expected now Jim Albers, Dave Samuels, Steve Rau and Peter Jenniskens are upgrading the hardware and software environment at the existing CAMS networks.

Finally, Andres Plata Stapper used deep-learning tools to discover additional structure in the 2010-2016 shower data pre-assigned by Jenniskens, which in the near future is expected to improve and enrich the meteor shower assignment template. Also, David Holman is working to created a new stream finder tool to help improve the shower isolation from the sporadic background.

The CAMS data reduction automation will make it possible to expand and create new low-light video camera networks to facilitate a continuous global monitoring of night-time meteor shower activity. [More here]

2017 Perseids

2017, August 13 - Carl Johannink and Martin Breukers of CAMS BeNeLux report that some 1070 meteors were captured during the peak of the Perseid meteor shower, with the results from some cameras still expected to come in after the observers have returned from vacation.

2017, August 8 - Peter Jenniskens finished the shower assignments, enabling Ian Webster to update the CAMS shower vizualisation tool to include all CAMS data up to the end of 2016. Many of the minor meteor showers are now well depicted.

2017, July 30 - Tim Cooper reports that the new CAMS South Africa network operated successfully. Data analysis shows that 167 meteors were captured simultaneously by the four cameras at Bredell and the four at Victory Park. Aside from many Southern delta Aquariids, there was a diffuse activity around R.A. = 20, Dec. = -15 degrees, and a compact radiant around R.A. = 40, Dec. = -32. No meteors from the Borisov trail were captured. Visual observations suggested a hint of activity later in the night. Peter Jenniskens, Mike Koop and Marcelo de Cicco observed the moon for possible impacts from California.

Lunar impacts

2017, July 29 - Peter Zimnikoval writes that the dust trail encounter with comet C/2015 D4 (Borisov) may also cause a noticeable uptick of lunar impact flashes if there are enough large meteoroids in the trail. He writes: "Of course, no one knowns if particles in the stream will reach sizes to be detected this way." If it does, the Moon happens to be in a favorable geometry to see this, with best viewing at the longitude of the central USA. The trail will hit the Moon a little later than Earth. Train your telescope at the dark side of the Moon in the area dotted in the attached graph. Update: The moon will cross the Borisov trail on July 29, 01h16m UT, 0.9 hours after the Earth, according to calculations by Pete Gural.

2017, July 29 (00:22 UT) - Earth is about to travel through the 1-revolution dust trail of long-period (700 year) comet C/2015 D4 (Borisov). Borisov Only about once every 25 years is such an intermediate long-period comet discovered that passes close enough to Earth's orbit to have dust trail encounters. This one passed perihelion in 2014. On July 29 at 0h22m UT, we are crossing the trail just behind the comet and near the center on the inside [Read more: CBET], both favorable conditions for meteor activity. However, we do not know if the comet was active in the previous return. No annual shower is known from this comet. If meteoroids were released, the shower may be visible from South Africa, radiating from the constellation Columba near the horizon in the south east.
[Picture of the comet, courtesy of G. Borisov]

SA first light

2017, July 23 - First light tonight for the CAMS South Africa network. 87 meteoroid orbits!! Network coordinator is Tim Cooper, former director of the Meteor Section of ASSA, who operates four Watec Wat902H cameras from Bredell, a suburb of Johannesburg. Four more cameras are operated by Oleg Toumilovich from Victoria Park, at a distance of 31 km. Setup support was provided by Steve Rau. Stations are ready for the upcoming encounter with the dust trail of comet C/2015 D4 (Borisov) on July 29.

FDL team

2017, June 26 - The Frontier Development Lab has started its activities. The FDL Comet Team that will work to automate the CAMS data processing consists of (from left to right): Susana Zoghbi, Antonio Ordonez, Andres Plata Stapper, and Marcelo de Cicco. They will work on deep-learning tools to filter and process the data. In addition, Jack Collison will provide support with the data processing automation. Pete Gural (CAMS software) and Siddha Ganju (Deep Learning techniques) are the technical mentors.



[News archive]


SETI Institute logo Curator: Peter Jenniskens
Responsible NASA Official: Lindley Johnson (NEOO)

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