[meteorite-list] Meteorite Picture of the Day
Today's Meteorite Picture of the Day: Dhofar 310 TS Contributed by: Peter Marmet http://www.tucsonmeteorites.com/mpodmain.asp?DD=02/20/2016 __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
Re: [meteorite-list] NASA Invites Public to Send Artwork to an Asteroid (OSIRIS-REx)
Greetings Meteorite_list friends! If you missed the chance to send your name to Bennu, here is another opportunity to extend your reach beyond Earth! Consider submitting one of your microscope images as inspiration for exploration, fireball photo or maybe a nice scene that inspired you while out in field hunting for meteorites. Note that all artistic expression is welcome. I seem to recall some poets on the meteorite-list. Best regards, Dolores Hill On 2/19/2016 4:08 PM, Ron Baalke via Meteorite-list wrote: February 19, 2016 RELEASE 16-019 NASA Invites Public to Send Artwork to an Asteroid NASA is calling all space enthusiasts to send their artistic endeavors on a journey aboard NASA's Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft. This will be the first U.S. mission to collect a sample of an asteroid and return it to Earth for study. OSIRIS-REx is scheduled to launch in September and travel to the asteroid Bennu. The #WeTheExplorers campaign invites the public to take part in this mission by expressing, through art, how the mission's spirit of exploration is reflected in their own lives. Submitted works of art will be saved on a chip on the spacecraft. The spacecraft already carries a chip with more than 442,000 names submitted through the 2014 "Messages to Bennu" campaign. "The development of the spacecraft and instruments has been a hugely creative process, where ultimately the canvas is the machined metal and composites preparing for launch in September,' said Jason Dworkin, OSIRIS-REx project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "It is fitting that this endeavor can inspire the public to express their creativity to be carried by OSIRIS-REx into space." A submission may take the form of a sketch, photograph, graphic, poem, song, short video or other creative or artistic expression that reflects what it means to be an explorer. Submissions will be accepted via Twitter and Instagram until March 20. For details on how to include your submission on the mission to Bennu, go to: http://www.asteroidmission.org/WeTheExplorers "Space exploration is an inherently creative activity," said Dante Lauretta, principal investigator for OSIRIS-REx at the University of Arizona, Tucson. "We are inviting the world to join us on this great adventure by placing their art work on the OSIRIS-REx spacecraft, where it will stay in space for millennia." The spacecraft will voyage to the near-Earth asteroid Bennu to collect a sample of at least 60 grams (2.1 ounces) and return it to Earth for study. Scientists expect Bennu may hold clues to the origin of the solar system and the source of the water and organic molecules that may have made their way to Earth. Goddard provides overall mission management, systems engineering and safety and mission assurance for OSIRIS-REx. The University of Arizona, Tucson leads the science team and observation planning and processing. Lockheed Martin Space Systems in Denver is building the spacecraft. OSIRIS-REx is the third mission in NASA's New Frontiers Program. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages New Frontiers for the agency's Science Mission Directorate in Washington. For more information on OSIRIS-Rex, visit: http://www.nasa.gov/osiris-rex -end- __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list -- Dolores H. Hill Sr. Research Specialist Lunar & Planetary Laboratory Kuiper Space Sciences Bldg. #92 The University of Arizona 1629 E. University Blvd. Tucson, AZ 85721 http://www.lpl.arizona.edu/ OSIRIS-REx Asteroid Sample Return Mission Communication & Public Engagement Team Lead OSIRIS-REx Ambassadors program Co-lead OSIRIS-REx Target Asteroids! citizen science program Co-coordinator Target NEOs! observing program of the Astronomical League http://osiris-rex.lpl.arizona.edu/ http://osiris-rex.lpl.arizona.edu/?q=target_asteroids http://www.astroleague.org/files/u3/NEO_HomePage.pdf __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] Pluto's 'Hulk-like' Moon Charon: A Possible Ancient Ocean?
http://pluto.jhuapl.edu/News-Center/News-Article.php?page=20160218 Pluto's 'Hulk-like' Moon Charon: A Possible Ancient Ocean? February 18, 2016 Pluto's largest moon may have gotten too big for its own skin. Images from NASA's New Horizons mission suggest that Charon once had a subsurface ocean that has long since frozen and expanded, pushing out on the moon's surface and causing it to stretch and fracture on a massive scale. The side of Charon viewed by the passing New Horizons spacecraft in July 2015 is characterized by a system of "pull apart" tectonic faults, which are expressed as ridges, scarps and valleys - the latter sometimes reaching more than 4 miles (6.5 kilometers) deep. Charon's tectonic landscape shows that, somehow, the moon expanded in its past, and "like Bruce Banner tearing his shirt as he becomes the Incredible Hulk" - Charon's surface fractured as it stretched. Charon's outer layer is primarily water ice. When the moon was young this layer was warmed by the decay of radioactive elements, as well as Charon's own internal heat of formation. Scientists say Charon could have been warm enough to cause the water ice to melt deep down, creating a subsurface ocean. But as Charon cooled over time, this ocean would have frozen and expanded (as happens when water freezes), pushing the surface outward and producing the massive chasms we see today. This image focuses on a section of the feature informally named Serenity Chasma, part of a vast equatorial belt of chasms on Charon. In fact, this system of chasms is one of the longest seen anywhere in the solar system, running at least 1,100 miles (about 1,800 kilometers) long and reaching 4.5 miles (7.5 kilometers) deep. By comparison, the Grand Canyon is 277 miles (446 kilometers) long and just over a mile (1.6 kilometers) deep. The lower portion of the image shows color-coded topography of the same scene. Measurements of the shape of this feature tell scientists that Charons water-ice layer may have been at least partially liquid in its early history, and has since refrozen. This image was obtained by the Long-Range Reconnaissance Imager (LORRI) on New Horizons. North is up; illumination is from the top-left of the image. The image resolution is about 1,290 feet (394 meters) per pixel. The image measures 240 miles (386 kilometers) long and 110 miles (175 kilometers) wide. It was obtained at a range of approximately 48,900 miles (78,700 kilometers) from Charon, about an hour and 40 minutes before New Horizons' closest approach to Charon on July 14, 2015. __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] NASA Invites Public to Send Artwork to an Asteroid (OSIRIS-REx)
February 19, 2016 RELEASE 16-019 NASA Invites Public to Send Artwork to an Asteroid NASA is calling all space enthusiasts to send their artistic endeavors on a journey aboard NASA's Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) spacecraft. This will be the first U.S. mission to collect a sample of an asteroid and return it to Earth for study. OSIRIS-REx is scheduled to launch in September and travel to the asteroid Bennu. The #WeTheExplorers campaign invites the public to take part in this mission by expressing, through art, how the mission's spirit of exploration is reflected in their own lives. Submitted works of art will be saved on a chip on the spacecraft. The spacecraft already carries a chip with more than 442,000 names submitted through the 2014 "Messages to Bennu" campaign. "The development of the spacecraft and instruments has been a hugely creative process, where ultimately the canvas is the machined metal and composites preparing for launch in September,' said Jason Dworkin, OSIRIS-REx project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "It is fitting that this endeavor can inspire the public to express their creativity to be carried by OSIRIS-REx into space." A submission may take the form of a sketch, photograph, graphic, poem, song, short video or other creative or artistic expression that reflects what it means to be an explorer. Submissions will be accepted via Twitter and Instagram until March 20. For details on how to include your submission on the mission to Bennu, go to: http://www.asteroidmission.org/WeTheExplorers "Space exploration is an inherently creative activity," said Dante Lauretta, principal investigator for OSIRIS-REx at the University of Arizona, Tucson. "We are inviting the world to join us on this great adventure by placing their art work on the OSIRIS-REx spacecraft, where it will stay in space for millennia." The spacecraft will voyage to the near-Earth asteroid Bennu to collect a sample of at least 60 grams (2.1 ounces) and return it to Earth for study. Scientists expect Bennu may hold clues to the origin of the solar system and the source of the water and organic molecules that may have made their way to Earth. Goddard provides overall mission management, systems engineering and safety and mission assurance for OSIRIS-REx. The University of Arizona, Tucson leads the science team and observation planning and processing. Lockheed Martin Space Systems in Denver is building the spacecraft. OSIRIS-REx is the third mission in NASA's New Frontiers Program. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages New Frontiers for the agency's Science Mission Directorate in Washington. For more information on OSIRIS-Rex, visit: http://www.nasa.gov/osiris-rex -end- __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] Mars Odyssey THEMIS Images: February 8-19, 2016
MARS ODYSSEY THEMIS IMAGES February 8-19, 2016 o Dark Slope Streaks (08 February 2016) http://themis.asu.edu/zoom-20160208a o Ridges (09 February 2016) http://themis.asu.edu/zoom-20160209a o Hills and Channels (10 February 2016) http://themis.asu.edu/zoom-20160210a o Lonar Crater (11 February 2016) http://themis.asu.edu/zoom-20160211a o Kasei Valles (12 February 2016) http://themis.asu.edu/zoom-20160212a o Tempe Terra (15 February 2016) http://themis.asu.edu/zoom-20160215a o Ceraunius Fossae (16 February 2016) http://themis.asu.edu/zoom-20160216a o Rampart Crater (17 February 2016) http://themis.asu.edu/zoom-20160217a o Granicus Valles (18 February 2016) http://themis.asu.edu/zoom-20160218a o Olympica Fossae (19 February 2016) http://themis.asu.edu/zoom-20160219a All of the THEMIS images are archive here: http://themis.asu.edu/latest.html NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in co.oration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena. __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] Mars Rover Opportunity Update: February 3-9, 2016
http://mars.nasa.gov/mer/mission/status.html#opportunity OPPORTUNITY UPDATE: Taking Panoramic Views and Prepping for Science - sols 4276-4282, February 03, 2016-February 09, 2016: Opportunity is exploring 'Marathon Valley' on the rim of Endeavour crater. The rover is up on very steep slopes to reach high-value science targets on 'Knudsen Ridge.' For the past week, Opportunity has been collecting extensive Pancam panoramas of the location all around Knudsen Ridge. One important purpose is to collect detailed imagery of the surface targets that the rover will approach next for detailed in-situ (contact) investigation. As of Sol 4282 (Feb. 9, 2016), the solar array energy production was 493 watt-hours with an atmospheric opacity (Tau) of 0.443 and a solar array dust factor of 0.675. Total odometry is 26.51 miles (42.66 kilometers), more than a marathon. __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] Trace Gas Orbiter and Schiaparelli Are Joined (ExoMars 2016)
http://exploration.esa.int/mars/57387-united-they-stand-trace-gas-orbiter-and-schiaparelli-are-joined/ United they stand - Trace Gas Orbiter and Schiaparelli are joined European Space Agency 16 February 2016 The Trace Gas Orbiter and Schiaparelli are now in their launch configuration. The ExoMars 2016 spacecraft will remain united until 16 October, when the entry, descent and landing demonstrator module will separate from the orbiter to descend to the surface of Mars. The mating of the Trace Gas Orbiter and Schiaparelli began on Friday 12 February with the two spacecraft having been transferred into the fuelling area, where a mounting platform surrounding the orbiter facilitates the activities that need to be done about 4 m off the ground. TGO and Schiaparelli are mechanically linked with the main separation assembly (MSA), which attaches to TGO with 27 screws. The MSA holds onto Schiaparelli with three separation mechanisms comprising compressed and angled springs that are held by non-explosive actuators (NEA). When the NEA's are released on 16 October, as the spacecraft approaches Mars, Schiaparelli will be gently pushed away from TGO, at the same time being imparted with a rotation that will serve to stabilize its atmospheric entry. Although this was the third time the two spacecraft have been mated - the previous occasions being in Cannes during integration and testing - it was the first time it was done with Schiaparelli fuelled, which required extra safety precautions to be applied. The next day, Saturday 13 February, all the electrical connections between the two spacecraft were made, which meant that some functional checks could also be started. These checks, which provide a means of monitoring that all systems are behaving as expected and that no problems have been introduced by any of the preparations, continued throughout the weekend and were completed on Monday 15 February. Meanwhile, on Sunday, specialists from the Airbus Defence and Space team began their preparations for bonding the last few tiles on Schiaparelli. Although most of the tiles had been placed and sealed last week, a few places on the heat shield had remained 'open' since these were the sites of hooks for the equipment that is used to lift Schiaparelli into place on the TGO. With this task completed the hooks could be removed and the final tiles placed and sealed. These will be finalized on Wednesday 17 February. (The bonding of the tiles requires some days to allow the bonding agent to cure before the final, finishing touches can be applied.) This week, on Tuesday and Wednesday, TGO and Schiaparelli will 'phone home': they will be connected (via the Network Data Interface Unit (NDIU)) to the mission operations centre at the European Space Operations Centre (ESOC), to run the last of the system verification tests (SVT-2b) on the spacecraft. By the end of the week, the spacecraft will be ready for fuelling of the Trace Gas Orbiter. __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] How the Sun Protects Earth from Asteroid Impacts
https://www.helsinki.fi/en/news/asteroids-are-not-destroyed-in-an-impact-with-the-sun Asteroids are not destroyed in an impact with the Sun University of Helsinki February 18, 2016 Puzzling asteroid and meteor observations can now be explained. For two decades it was thought that most near-Earth objects (NEOs) end their existence in a dramatic final plunge into the Sun. A new study published in the journal Nature finds instead that most of those objects are destroyed much farther from the Sun than previously thought. This surprising new discovery explains several puzzling asteroid and meteor observations that have been reported in recent years. - Initially our aim was to construct a state-of-the-art model of the NEO population that is needed for planning future asteroid surveys and spacecraft missions, says planetary scientist Mikael Granvik, currently at the University of Helsinki. The best-ever model The model that describes the NEOs' orbit and size distributions was completed as planned, but the research also led to an important advance in asteroid research. - We modelled different observational selection effects, and combined them with observational data and NEOs' well-understood, statistical orbit distributions that vary depending on an NEO's specific source region in the main asteroid belt. But the team noticed that their model had a problem: the number of NEOs detected was 5 per cent less than the model predicted. They then spent a year verifying their calculations before they came to the conclusion that the problem was not in their analysis but in their assumptions of how the Solar System works. The model was then modified to the new hypothesis that NEOs are destroyed if they spend too much time within about 10 solar diameters of the Sun, and this lead to an excellent agreement between the model and the observed population of NEOs. Why some meteor streams lack parent objects The team's discovery helps to explain several other discrepancies between observations and predictions of the distribution of small objects in our Solar System. - Astronomers have been unable to match most of the meteor streams on orbits closely approaching the Sun with known parent objects, says Granvik. He and his research team now suggest that the parent objects were completely destroyed when they came too close to the Sun. The team can now also explain why NEOs that approach closer to the Sun are brighter than those that keep their distance from the Sun. Darker asteroids are more easily destroyed - Darker asteroids that have been orbiting closer to the Sun have already been destroyed. The fact that dark objects are more easily destroyed implies that dark and bright asteroids have a different internal composition and, possibly, structure. According to Granvik, their discovery of the catastrophic loss of asteroids before a collision with the Sun allows planetary scientists to understand a variety of recent observations from a new perspective. - Perhaps the most intriguing outcome of this study is that it shows that it shows that one must account for the asteroids' physical properties when constructing population models. - In simple terms one can say that it is now possible to test models of asteroid interiors simply by keeping track of their orbits and sizes. This research led by Mikael Granvik is published in Nature, 18 February. __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] NASA Introduces New, Wider Set of Eyes on the Universe (WFIRST)
http://www.jpl.nasa.gov/news/news.php?feature=5371 NASA Introduces New, Wider Set of Eyes on the Universe Jet Propulsion Laboratory February 18, 2016 After years of preparatory studies, NASA is formally starting an astrophysics mission designed to help unlock the secrets of the universe -- the Wide Field Infrared Survey Telescope (WFIRST). With a view 100 times bigger than that of NASA's Hubble Space Telescope, WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life. NASA's Agency Program Management Council, which evaluates the agency's programs and projects on content, risk management and performance, made the decision to move forward with the mission on Wednesday. The mission is led by NASA's Goddard Space Flight Center in Greenbelt, Maryland. NASA's Jet Propulsion Laboratory in Pasadena, California, will manage the mission's 7.8-foot (2.4-meter) telescope and deliver the coronagraph, an instrument to help image and characterize planets around other stars. The Infrared Processing and Analysis Center (IPAC) at the California Institute of Technology in Pasadena will share science center activities with the Space Telescope Science Institute in Baltimore, under Goddard leadership. "WFIRST has the potential to open our eyes to the wonders of the universe, much the same way Hubble has," said John Grunsfeld, astronaut and associate administrator of NASA's Science Mission Directorate at Headquarters in Washington. "This mission uniquely combines the ability to discover and characterize planets beyond our own solar system with the sensitivity and optics to look wide and deep into the universe in a quest to unravel the mysteries of dark energy and dark matter." WFIRST is the agency's next major astrophysics observatory, following the launch of the James Webb Space Telescope in 2018. The WFIRST observatory will survey large regions of the sky in near-infrared light to answer fundamental questions about the structure and evolution of the universe, and expand our knowledge of planets beyond our solar system - known as exoplanets. It will carry a Wide Field Instrument for surveys, and a Coronagraph Instrument designed to block the glare of individual stars and reveal the faint light of planets orbiting around them. By blocking the light of the host star, the Coronagraph Instrument will enable detailed measurements of the chemical makeup of planetary atmospheres. Comparing these data across many worlds will allow scientists to better understand the origin and physics of these atmospheres, and search for chemical signs of environments suitable for life. "WFIRST is designed to address science areas identified as top priorities by the astronomical community," said Paul Hertz, director of NASA's Astrophysics Division in Washington. "The Wide-Field Instrument will give the telescope the ability to capture a single image with the depth and quality of Hubble, but covering 100 times the area. The coronagraph will provide revolutionary science, capturing the faint, but direct images of distant gaseous worlds and super-Earths." The telescope's sensitivity and wide view will enable a large-scale search for exoplanets by monitoring the brightness of millions of stars in the crowded central region of our galaxy. The survey will net thousands of new exoplanets similar in size and distance from their star as those in our own solar system, complementing the work started by NASA's Kepler mission and the upcoming work of the Transiting Exoplanet Survey Satellite. Employing multiple techniques, astronomers also will use WFIRST to track how dark energy and dark matter have affected the evolution of our universe. Dark energy is a mysterious, negative pressure that has been speeding up the expansion of the universe. Dark matter is invisible material that makes up most of the matter in our universe. By measuring the distances of thousands of supernovae, astronomers can map in detail how cosmic expansion has increased with time. WFIRST also can precisely measure the shapes, positions and distances of millions of galaxies to track the distribution and growth of cosmic structures, including galaxy clusters and the dark matter accompanying them. "In addition to its exciting capabilities for dark energy and exoplanets, WFIRST will provide a treasure trove of exquisite data for all astronomers," said Neil Gehrels, WFIRST project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "This mission will survey the universe to find the most interesting objects out there." Twelve science investigation teams were recently selected by NASA to help optimize science returns for the mission. Olivier Doré of JPL leads one of the teams. His group will focus on co
[meteorite-list] AD1 2016 (free ad) - Some nice NWA slices on Ebay
Dear list members I'm offering very nice slices of different NWA meteorites on Ebay. Low TKW, low starting bid, no reserve auctions. Ending coming Sunday. More to come, so have a look again in the coming weeks. NWA 6057 (prov.) Achondrite) NWA 6475 (Eucrite pmict) NWA 8310 (Chondrite LL5-7) NWA 8377 (Chondrite CV3) next week: NWA 5995 (Achondrite polym. with nano diamonds) NWA 6059 (Chondrite L6) NWA 6476 (Chondrite IMB H5) http://stores.ebay.com/SAHARAGEMS-Meteorites-and-more?_rdc=1 Thanks for looking. Thomas saharag...@yahoo.com IMCA 8629 __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
[meteorite-list] Southern France / Italy Bolide Fireball Meteor 18.20 (GMT +1) 17FEB2016 w/ Videos
List, Southern France / Italy Bolide Fireball Meteor 18.20 (GMT +1) 17FEB2016 w/ Videos MeteorRats Scramble! Booms reported with smoke trail. Rocks?! http://lunarmeteoritehunters.blogspot.jp/2016/02/france-italy-bolide-fireball-meteor.html Dirk Ross...Tokyo The Latest Worldwide Meteor/Meteorite News http://lunarmeteoritehunters.blogspot.com/ __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
Re: [meteorite-list] Arizona Fireball Meteor 06:35am MST 15FEB2016
Hi List, That's funny. I saw that Fireball. I was driving in tucson from my Hotel to the show. That was a huge one, and I think it fell near of Tucson because it ended up before the mountains. Mohammed HMANI I.M.C.A #0153 www.sahara-nayzak.com Le 15 févr. 2016 à 16:17, drtanuki via Meteorite-list a écrit : > List, > > Arizona Fireball Meteor 06:35am MST 15FEB2016 > http://lunarmeteoritehunters.blogspot.jp/2016/02/arizona-fireball-meteor-15feb2016.html > > > Dirk Ross...Tokyo The Latest Worldwide Meteor/Meteorite News > http://lunarmeteoritehunters.blogspot.com/ > __ > > Visit our Facebook page https://www.facebook.com/meteoritecentral and the > Archives at http://www.meteorite-list-archives.com > Meteorite-list mailing list > Meteorite-list@meteoritecentral.com > https://pairlist3.pair.net/mailman/listinfo/meteorite-list __ Visit our Facebook page https://www.facebook.com/meteoritecentral and the Archives at http://www.meteorite-list-archives.com Meteorite-list mailing list Meteorite-list@meteoritecentral.com https://pairlist3.pair.net/mailman/listinfo/meteorite-list
