by Robert Verish
The Southern African Meteorite Recovery Program
This months article is about the Southern African Meteorite Recovery Program (SAMRP) and its place in history in regards to meteorite-recovery.....
While doing a Google search on "meteorite-recovery", I discovered that there has been an M-R effort underway by a small group of Southern African astronomers since 1999!
It appears that an awareness of a need for an organized approach to meteorite-recovery in the field by utilizing the group efforts of "non-professionals" seems to have taken root in the Southern African astronomy community along about the same time period as similar efforts were producing results here in Southern California!
The founder of this group, Trevor Gould, stated that, "Following the 62nd Meeting of the Meteoritical Society at
University of the Witwatersrand in July 1999, I got to thinking about the role of amateurs and the recovery of meteorites." What resulted was his "Notes on Proposed Meteorite Recovery Program for Southern Africa", which became the start ot the SAMRP. The rest, as they say, "is history"! See for yourself in the web pages reproduced below.
[Just as an aside for historical accuracy, it may be more than coincidental that I presented a poster at this very same 62nd Meeting of the Meteoritical Society. So, please excuse me then, if I rationalize that my unassuming poster (by a "non-professional") with images of successful meteorite recoveries at Lucerne Dry Lake, may have given others the idea that, "Hey, I can do that, too!"]
;-)
It is the hope of this article that the recounting of the successes (as well as as the shortcomings) of the formation and the evolution of the SAMRP will be instructional for other fledgling Meteorite-Recovery groups.
The following tables are various web pages of the "Southern African Meteorite Recovery Program" which have been reproduced here for readers convenience, as well as, to retain for historical purposes, its importance in the development of meteorite-recovery in Southern Africa.
Notes on Proposed Meteorite Recovery Program for Southern Africa - 1999
The webmaster for all of the following web pages is Trevor Gould:
Meteorite Recovery in Southern
Africa
We have all seen and enjoyed watching meteors
rushing dramatically across the night sky. If we have been fortunate and observant [I
havent], we may have seen a daylight meteor.
Once a small chunk of interplanetary rock reaches the surface of the Earth it ceases to be a meteor and becomes a meteorite. The recovery, preservation and study of meteorites is an important prelude to assembling the early the history of the Solar System. Im not going to write about meteors, because Tim Cooper does that excellently. Im also not going to write about the history of the Solar System, despite it being one of my major interests. I intend to write to write about the recovery of meteorites in Southern Africa, but if I wander off the subject a little, I hope you will forgive me. In July 1999, South Africa hosted the 62nd Annual Meeting of the Meteoritical Society, an international inter-disciplinary body [see my other article in MNASSA] dedicated to a fairly range of planetary sciences, including the recovery and study of meteorites. Up to now, the recovery of meteorites has been either a serendipitous process, resulting from seeing a fall, finding a large and unmistakable meteorite, or a short term project to find anything that may have fallen in a likely spot. Following the 62nd Meeting of the Meteoritical Society at University of the Witwatersrand in July 1999, I got to thinking about the role of amateurs and the recovery of meteorites. I also did some initial enquiries and put together an informal proposal which I sent off to Professor Wolf Uwe Reimold at the Department of Geology, U Wits. I considerd that this could be an ideal activity for amateurs to be involved in, and that the Johannesburg Centre would be an ideal body to run with the concept. The initial proposal, rushed off before the results of the first enquiries were available was a little off the mark, but, nevertheless, here it is:
Notes on Proposed Meteorite Recovery Program for Southern Africa
Pilot Project- Silver Streams Professor Reimold accepted the proposal, and we set up a pilot project to test the concept feasibility. Without using anything more high tech than a road map which showed a pan close to the road near Silver Streams, I managed to obtain the names and contact details for farmers who owned pieces of pan, and obtained permission to conduct a recovery operation on those parts [one farmer refused to grant permission over the weekend, another two accepted and one of those offered overnight accommodation]. Brian and Val Fraser and I conducted a search in September. We had considered that the chief problem may be heat and sun and we were indeed fortunate not to have to deal with that problem at all, as it had snowed in the vicinity overnight and the temperature was, taking wind chill into account, only just above freezing. Just as I had hoped, a fair area of pan was free of vegetation, although much was covered with a short grass. Additionally, the bare area consisted of a light coloured calcrete, against which it was hoped that the black fusion crusts of meteorites would stand out in profusion. Sure enough, a large number of black objects did stand out in profusion, but they all turned out to be the weathered remains of loose pieces of the underlying Transvaal Dolomite, which weathers to a black colour. With such a low signal to noise ratio, no meteorites were recovered. Subsequent Progress A number of meteoriticists have provided useful information:Dr Mike Zolensky [JSC, NASA] has advised that many meteorites in the Namib weather to a red/brown, not black. Dr Sara Russell of the Natural History museum in London has also advised on legalities of collecting in Namibia, and also likely areas. Dr Alex Bevan, curator of meteorites in Western Australia, has also helped with information on the 15 years of recovery operations he conducted in the deserts of Western Australia. In addition, he advised that in Australia searches are successfully conducted amongst the piles of stones farmers gather at the edge of fields. They all wish us well. Professor Reimold is concerned that we need to be less random in the selection of likely locations and to this end has suggested a meeting with a sedimentologist, Dion Brandt, of Wits Geology. This meeting identified bare areas of low sedimentation and high ablation that should multiply our chances of recovery. The low sedimentation principle means that meteorite falls will not be covered rapidly by sand/ mud etc., and will remain exposed longer. The high ablation principle suggests that if a meteorite did become buried [and some meteorite are quite capable of digging holes!] the covering material will be blown away by wind [or washed away] to expose the underlying meteorite. The longer the time interval [the Kalahari is some 80 million years old], the more meteorites it will have soaked up, and the better the chances of recovering one or more. The improved chances are however, offset by the high rate of weathering of meteorites, which, for stony meteorites makes them unidentifiable within a year. Professor Reimold is also willing to conduct a training course for interested people who do not know how to identify a meteorite. Team Members Initially, we will restrict recovery team members to members of the Johannesburg Centre, but hopefully as the operation grows, we can include members of other centres, students and interested members of the general public.If the operation does take off, it may provide a source of new members. There are some costs, and these can be quite considerable. The first cost is transportation to the remote site [ meteorites seldom fall conveniently close to home], and the second is accommodation [we cannot rely on the goodwill of farmers]. Basic equipment is more than likely to hand anyway. Team member functions include organisation [setting up an expedition], site selection, obtaining the names of owners of the site and obtaining permission from them to recover meteorites, photography of the meteorite before it is recovered, administration [assigning an initial unique identifier to the recovery], provision of transport, finding accommodation locally, handing the finds over to the University for study, obtaining feedback etc., catering on site, etc. We also need someone with knowledge of first aid. Whatever you can contribute will be used in some way and will be most welcomed. Here is another unusual opportunity for we amateurs to contribute to science. If anyone would like the opportunity to get out of the city into the country for, probably, a weekend [the distance one can go is limited by the length of the weekend and the balance between search time and travel time], please contact:
Trevor Gould Home: 011-886-5602 |
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As a personal preference, I find the word "non-professional" more appealing than "amateur". But this "proposal" seems to show that this group effort is off to a very good start!
It wasn't until two years later that the SAMRP conducted a survey of the Vaalputs National Nuclear Waste Disposal site about 100Km SE of Springbok in the Northern Cape. It has long been an idea of mine to have meteorite-recovery as part of any environmental impact study (EIR) - to be included with the archeological, paleontological and other surveys - especially for large tracts of barren land that will be rendered lost due to development. In this particular case, the site was barren, but it was also very sandy. Although no meteorites were recovered, their thorough report shows a great deal of effort is starting to show progressive results.
Deo Gloria Members
Thanks also go to the Department of Geology, University of the Witwatersrand, for general and specific assistance with the expedition and its objective. We would also like to thank Dr Paul Buchanan, a professional meteoriticist, for taking time out to come along and share his expertise with us. The staff of NECSA [Nuclear Energy Corporation of South Africa] are also thanked for their kind assistance, especially Dr Marco Andreoli [Pelindaba], Kobus Byleveld [Manager:Vaalputs Facility], and Rhona who went out of her way to make our expedition one to remember, by providing a guided tour of the facility and local sights. Expedition Area The expedition search area was defined by Dr Dion Brandt to be the Vaalputs National Nuclear Waste Disposal site about 100Km SE of Springbok in the Northern Cape.A large scale satellite image was made available. This was scanned and used in situ. Site Description Vaalputs is a large site [about 20Km on the long side] area split by a public road. The area to the West of the road [Garies] moves westward into mountains and includes the accommodation facilities. 1:50000 map number is 3018 Loeriesfontein.The area to the East of the road is low lying [possible graben] in which sand has accumulated over a long period of time. Owing to strong winds the dune heights are low [about 5m], with a wavelength of about 500m. The wind ablation has scoured the place, presumably leaving any meteorites on the dune surfaces. The Waste disposal site is also here. Owing to the featureless nature of the terrain here, AEC recommend the use of a GPS. Itinerary
The philosophy has always been to have an enriching experience first, something to remember, and not to focus exclusively and exhaustively on meteorite hunting, and the value of that approach proved itself once again. Spring, 2001 The next expedition will take place in a dune field North of Upington, but South of the Kalahari Gemsbok National Park. Dates will be announced closer to the time.Trevor Gould |
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Again, another thorough report showing continued progress. But the great support that this group is getting from the various local professionals, now more than ever begs the question, "Why no recovered meteorites from this part of Africa by this well-supported group, when during the same time period there are so many finds reported in the Meteoritical Bulletin (No.86) just alone from the Southwestern USA?
2001.06.03 September 2001 Expedition Members
Results More samples were returned to the University of the Witwatersrand for analysis than on the previous expedition. Of these three proved to be worthy of further analysis and Professor Uwe Reimold and Dr Paul Buchanan called for thin sections to be made. Unfortunately, they all proved to be volcanics. Acknowledgments and thanks The team wish to thank the South African Heritage Resources Agency for kindly providing a permit to collect any meteorite finds in specific areas, and especially Ms Mary Leslie. Thanks also go to the Department of Geology, University of the Witwatersrand, for general and specific assistance with the expedition and its objective. The location was clarified by Professor Bernie Moon: our thanks go to him for taking the time to help us. We would also like to thank Stephan Laubscher, a professional geologist, for taking time out to come along and share his expertise with us. Thanks are also conveyed to the Council for Geoscience, both in Pretoria and Upington, for assistance rendered. Expedition Area The search area was defined as the set of permanent dunes North of Upington and South of the Kalahari Gemsbok Park. The intention was to find locations with minimal sand, such that inter-dune areas would be essentially desert pavement and to search the inter-dune areas. The logic of this approach was that even permanent dunes move slowly and that as they move they would absorb any meteorites and eventually deposit them on the trailing edge: i.e. the desert pavement. Site Description The inter-dune areas seen were extensively vegetated, and included thick sand cover. The dunes were vegetated to a higher degree than expected, but it would have been unlikely to find other than fresh falls on dune surfaces anyway. Therefore searches were restricted to dry pan surfaces, of which there were a number in the vicinity. The pans were of two types the most common surface was covered in gravel and boulders related to erosion of Dwyka tillite, while less commonly we found salt encrusted surfaces with similar Dwyka tillite erosional remains. The Dwyka represents a period of continental glaciation in South Africa, and this means that the provenance of the remains was generally far distant and of widely different rock types. This provided a rich source of many different rock types, which also had the effect of reducing the signal to noise ratio hoped for: many rocks had magnetic signatures, and demonstrated expected meteoritic features. A reasonably large number showed black fusion crusts which proved to be desert patina. One even had a radial flow pattern on one side of a rounded dark rock, which looked just like and oriented meteorite: the radial pattern resulted from radiating dolomite crstals! Another dark rock lay on the white salt surface [Norokei Pan] and showed regmaglypt features characteristic of iron meteorites: it is magnetic, heavy, but proved to be terrestrial. On one salt pan [Wit Pan] which was relatively devoid of any rocks a number of tiny greenish rocks were found in what appeared to be a strewn field pattern: they were magnetic, but proved to be weathered lavas. Expedition Diary
Comment Despite the lack of success, we built some local knowledge and experience of the art of meteorite hunting. Given one recoverable meteorite per grid 10Kms on a side, we would be within 5Km of one if we stood in the middle of the grid. This looks easy, but lets look a little more deeply. A searcher can successfully scan 2.5m on either side and therefore searchers are spread 5m apart. On a 10Km side, there are 2000 search lines, each 10Km long. To find one recoverable meteorite, expect to walk 20 000Kms! The grid of 100 square km. is also slightly optimistic, as the Saharan experience is one meteorite per 200 square Km. Again, you assume that your under-trained searcher will recognise a meteorite after walking in the hot sun all day. I am not surprised we have found nothing as yet, but the only place where success comes before work is in the dictionary. Therefore: Spring 2002 For the Spring Expedition, well be returning to the Upington / Kalahari Gemsbok district. The Expedition will be paired with a Deep Sky Observing Expedition, again under the auspices of the Johannesburg Centre. Dates are: Good Friday 29 March to Sunday 7 April. Hope you join us for this exciting Kalahari Safari! Trevor Gould |
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Again, another thorough report. It has been very interesting reading the various assumptions that have been written in these various web pages. The above "Comments" section was very insightful. The conclusions that have been drawn - to explain the lack of finds up to now - are quite at odds to the observations made by field workers here in the Southwestern USA. In time, if these disparities continue, it may become important to reconcile these differences. There could be something of importance to be learned.
And finally, here is the latest SAMRP web page, to the best of my knowledge, but so far there has been no follow-up to the results of this proposed meteorite recovery field trip.
Deo Gloria Post-Easter 2003 Expedition You are invited to join the post-Easter 2003 Expedition to the Kalahari semi-desert, North of Upington, to search for historic meteorite falls. Dates: Saturday 26 April to Sunday 4th May [or part thereof]. Volunteers who are prepared to assist with the search for meteorites are requested to contact the writer for further information. Those who would simply enjoy joining the expedition in order to observe from exceptionally dark skies are also welcome. Note: while it may be possible to stay at or near a Bed n Breakfast establishment, it may prove necessary to camp in remote area with no access to ablution facilities. Volunteers need to be fit to walk the expected distances. No medical facilities will be available. The timing is intended to fall between the cold of winter and the heat of summer, however, the week away could well see heat, cold, wind and rain. Nights are usually cold, but clear, and telescopes for star viewing will be brought along. Note that electrical power is unlikely to be available on campsites. Roads are usually suitable for ordinary sedan vehicles: bakkies or 4X4s, while useful, should not be necessary. For those able to come, there will be a workshop covering both procedure / logistics of the Expedition and Field Recognition of Meteorites to be held at the Observatory 18a Gill Street, Observatory, Johannesburg at 20:00 Friday 11 April 2003. We hope that some real meteorites will be available at the workshop. This workshop will also provide a sample list of things to bring, including food, water, camping equipment, medicals etc. Meteorite hunting equipment will be available. The Itinerary shown is subject to change. Itinerary for Meteorite Hunters
Trevor Gould |
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From Ron Baalke
Workshop on Extraterrestrial Materials from Cold and Hot Deserts
http://www.lpi.usra.edu/meetings/metsoc99/metsoc99.2nd.html#WORKSHOP
Where, When, and What
The Workshop on Extraterrestrial Materials from Hot and Cold Deserts
will take place in the Kwa-Maritane Resort in the Pilanesberg Game
Reserve, about 130 km northwest of Johannesburg from July 6 to 8,
1999 prior to the Meteoritical Society Meeting in Johannesburg.
It is planned to leave Johannesburg by bus on July 6th (about noon)
and return on July 8th in the evening. This schedule will allow
those attending to participate in the Vredefort excursion prior to
the MetSoc `99 meeting.
This Workshop aims at bringing together persons working with
meteorites or micrometeorites found in the Arctic, the Antarctic,
and in hot deserts. Talks and posters (if the number of submitted
presentations is more than about 30) on the following topics are
welcome:
- new meteorite searches and their results
- unique or rare types of meteorites
- weathering effects of meteorites and implications
- differences between desert meteorites and modern falls
- cosmogenic nuclides and age distributions
- comparisons between micrometeorites and IDPs collected in the stratosphere
- collections, handling, consortia
Call for Abstracts
Similar to previous Workshops on this topic we plan to publish
extended abstracts (up to 5 pages) in the form of a LPI Technical
Report. Please submit your abstract to Ludolf Schultz before May 15,
1999 as a hard copy and a Word file. After the meeting the abstract
can be revised and the final version will then be due on Sept. 15,
1999.
FULL DETAILS at:
http://www.lpi.usra.edu/meetings/metsoc99/metsoc99.2nd.html#WORKSHOP
The topic of my next few articles will continue a series on California and Nevada Meteorites.
My previous articles can be found *HERE*
For for more information, please contact me by email:
Bolide*chaser
Pilanesberg, South Africa
July 6 - 8, 1999