Many meteorites with the potential for a photographic orbit have fallen since I started this page. They all go into my candidate list, and I regularly check whether any of them have been published in the mean-time. However, the process is not perfect, as the case of Ozerki demonstrates: Ozerki is an L6 that fell in June 2018 in Russia. Its orbital elements have been published by Kartashova et al. in 2020 in Planetary and Space Science, and yet, I never stumbled over the paper. Anyway, Ozerki is in the database now. If you know of any other meteorites that I missed, please let me know.
Kyrylenko et al. report in an LPSC abstract (PDF) that they might have found the first iron meteorite with an orbit. The still unnamed, unofficial meteorite (at time of checking the MetBull database on May 24th, 2022) with a mass of 13.7 kg fell on November 7th, 2020, and seems to have a determined orbit with rough parameters of a = 1.9 AU and e = 0.5. More details are certainly forthcoming in a future publication, at which point I will include the orbit on the list.
An iron meteorite with an orbit is a very welcome and exciting addition to the suite of meteorites with orbits. Irons make out only about 4% of all falls, so “it’s about time” we have one among the 40 orbits known today. While the orbital parameters given in the abstract do not look remarkably different, over time – with more iron meteorite orbits to be expected in the future – the picture of iron meteorite origins will become much clearer. /m4
Vida et al. have published an abstract (PDF) to the European Planetary Science Congress (EPSC) of 2021 where they give the orbital parameters for Novo Mesto, an L5 chondrite with a photographic orbit which fell in Slovenia in February 2020. This is enough for inclusion in our list of published meteorite orbits, and a corresponding entry has been added. In total, there are now 38 meteorites with published orbital elements derived from photographic documentation.
To answer a related frequently asked question, I am aware that there are a number of recently fallen meteorites for which it is known that orbital elements were determined based on photographic documentation of the entry fireball – however, the orbital elements for these meteorite orbits are not currently available in the scientific literature because the authors chose not to add them to an abstract where they announced the publication of an orbit solution, or just haven’t published them yet in a regular journal article. If you find an abstract or article reporting orbital elements for a meteorite currently not listed, please let me know. /m4
A new meteorite with associated orbit has been added to the table: Motopi Pan. Although officially classified as a howardite (in the MetBull database), it is a complex HED breccia with howardite, cumulate and basaltic eucrites, as well as diogenite lithologies, as the authors write in an article published online today in MAPS (Jenniskens et al., 2021). This is only the second time (the first was Almahata Sitta in 2008) that a meter-scale asteroid was found to be on a collision course with Earth only a few hours prior to impact (the asteroid was named 2018 LA), observed as a meteor when it entered the Earth’s atmosphere, and meteorites recovered afterwards, this time in Botswana. Because of the longer observation arc, the orbit is much better constrained compared to a typical “meteorite-with-orbit” fall. The orbit strongly suggests the meteoroid was delivered via the nu-6 resonance from the large asteroid Vesta. From the combination of ejection age (= cosmic-ray exposure age, ca. 22 Ma) and shock-reset age in phosphates, Jennsikens et al. (2021) even suggest that the source crater of the impact might be Rubria, in the Venenaia impact basin on Vesta.
Full disclosure: I am a co-author on the paper. /m4
The table of orbits and the three Figures (number and type of falls vs. year of fall, plane view of the solar system with all orbits, eccentricity vs. semi-major axis) have all been updated to include all 36 currently known meteorites with published photographic orbits. /m4
A paper describing the trajectory and orbit of the Flensburg (carbonaceous, C1 ungrouped) meteorite, which fell on September 12th, 2019 in northernmost Germany, has been accepted for publication into MAPS, and the corresponding preprint uploaded on arxiv.org. The meteoroid delivering the single known piece of the Flensburg meteorite (of only 24.5 g) originates from a quite elongated orbit with a large semi-major axis (ca. 2.8 AU), which puts it right on the 5:2 orbital resonance with Jupiter, as well as in the Jupiter Family Comets field (2 < Tisserand parameter <3). It had a mass in the range of 10-20 metric tons and correspondingly, a radius of 2-3 meters. The authors suggest that based on the orbit and the very short cosmic-ray exposure age of only 7 ka (Bischoff et al., 2021), the meteoroid probably originated on a carbonaceous asteroid close to the edge of the 5:2 resonance.
Flensburg is only the fourth carbonaceous meteorite with an orbit (the others being Tagish Lake, Maribo, and Sutter’s Mill). Its interesting to note that carbonaceous meteorites are now slightly over-represented (ca. 11%) among meteorites with orbits compared to their abundance among “normal” finds (ca. 4%), perhaps because, once landed on the surface, they decay quickly and are thus less likely to be found without the “prompt” provided by the fireball observation. /m4
A new paper by Gardiol et al. in MNRAS (available online) summarizes the results from the initial investigation of the Cavezzo chondrite, which fell in Italy on the evening of January 1st, 2020. The meteorite, of which two fragments have been found, is an anomalous L5 chondrite, the 9th L-chondrite out of 34 meteorites with orbits. The semi-major axis and eccentricity of its parent meteoroid plot along the characteristic trend, and as is often observed, the perihelion is just inside Earth’s orbit, while the aphelion is in the asteroid belt. /m4
A new meteorite with an orbit has been published in Meteoritics & Planetary Science (MAPS): Dishchii’bikoh. It is a rare LL7 chondrite which fell near the city of Cibecue in Arizona / USA, and takes its name as pronounced in the language of the local White Mountain Apache tribe. Several fragments of almost 80 g total mass were recovered using the weather radar footprint of the fall. The orbit of the meteorite is remarkable for being relatively short (1.13 AU semi-major axis) and steeply inclined (ca. 21° to the ecliptic). Radionuclides suggest it was a relatively large meteoroid, at R = 60-100 cm. The cosmic-ray exposure age is quite typical for an ordinary chondrite, at 11 Ma. It seems likely the meteorite derived from the Flora family of asteroids in the inner asteroid belt, similar to other recent LL chondrite falls, like Stubenberg (2016) and Chelyabinsk (2013).
Full disclosure: I am a co-author on the paper. /m4
In the morning of February 28th, a bright daytime fireball was observed over Slovenia. Now, a fresh, fusion-encrusted meteorite (ca. 200 g), looking like an equilibrated chondrite, has been found in the region where the fragments from the fireball were expected to drop. On March 7th, it was found and reported by Gregor Kos in the driveway of his house, and later confirmed to be a meteorite by Bojan Ambrozic. Later that same day, the meteorite was handed over to the Natural History Museum of Slovenia. The prospective name of the meteorite (not yet approved by the Meteoritical Society, which is why I provide the name with an asterisk) is Novo Mesto*.
Obviously, this is an excellent candidate for a meteorite which will have an associated orbit. /m4
On March 2nd, ca. 23:38 UTC (0:38 local, i.e., CET), a large fireball was observed over North-West Germany, as the IMO (International Meteor Organization) reports. At an estimated diameter of 2 meters and a mass of about 10 tons (although this is contingent on the assumed entry velocity of 14 km/s and the assumed density of 3000 kg m3). At that size and relatively slow velocity, it seems plausible that some meteorites survived, but again, this depends on the assumptions made. Any meteorites would have fallen to the south-east of the city of Wesel on the Rhine.
Of course, there many meteors falling all the time, but this one seems very well observed (165 observations accross multiple countries!) and also relatively large; furthermore, there are several films of the meteor captured from multiple angles – so it seems likely that in this particular case, if any meteorites are found, they will have a very well-defined orbit. We’ll see if anything interesting (in terms of meteorites, of course!) comes from this – until then, that meteor goes to the candidate list. /m4