The Meteoritical Bulletin, No. 113

Jérôme Gattacceca, Francis Mccubbin, Jeffrey Grossman, Devin Schrader, Camille Cartier, Guy Consolmagno, Cyrena Goodrich, Ansgar Greshake, Juliane Gross, Katherine Helen Joy, et al.

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Jérôme Gattacceca, Francis Mccubbin, Jeffrey Grossman, Devin Schrader, Camille Cartier, et al. The Meteoritical Bulletin, No. 113. Meteoritics and Planetary Science, 2025, 113, pp.1-5. 10.1111/maps.14374. hal-05101637

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Distributed under a Creative Commons Attribution 4.0 International License
The Meteoritical Bulletin, No. 113

Jérôme GATTACCECA<sup>1*</sup>, Francis M. McCUBBIN<sup>2</sup>, Jeffrey N. GROSSMAN<sup>3</sup>, Devin L. SCHRADER<sup>4,13</sup>, Camille CARTIER<sup>5</sup>, Guy CONSOLMAGNO<sup>6</sup>, Cyrena GOODRICH<sup>7</sup>, Ansgar GRESHAKE<sup>8</sup>, Juliane GROSS<sup>2,9</sup>, Katherine Helen JOY<sup>10</sup>, Bingkui MIAO<sup>11</sup>, and Bidong ZHANG<sup>12</sup>

*Correspondence

Jérôme Gattacceca, CNRS, Aix Marseille Univ, IRD, INRAE, CEREGE, Aix-en-Provence, France.

Email: gattacceca@cerege.fr

(Received 09 May 2025; revision accepted 19 May 2025)

**Abstract**—Meteoritical Bulletin 113 contains the 3646 meteorites approved by the Nomenclature Committee of the Meteoritical Society in 2024. It includes 17 falls, 2964 ordinary chondrites, 218 HED, 158 carbonaceous chondrites (including 7 ungrouped), 59 lunar meteorites, 38 iron meteorites (9 ungrouped), 30 ureilites, 31 primitive achondrites (3 ungrouped), 28 mesosiderites, 24 enstatite chondrites, 21 martian meteorites, 24 ungrouped stony achondrites, 20 Rumuruti chondrites, 17 pallasites, 8 angrites, 5 enstatite achondrites (one ungrouped), and 1 ungrouped chondrite. Of the meteorites approved in 2024, 1250 were collected in Antarctica, 1102 in Africa, 689 in Asia, 575 in South America, 17 in North America, 11 in Europe, and 2 in Oceania.

TRENDS AND SPECIFICITIES

Meteoritical Bulletin 113 (MB113) contains the 3646 meteorites submitted to and accepted by the Nomenclature Committee of the Meteoritical Society in 2024. This is the largest number ever registered by the Meteoritical Society in a calendar year since the Meteoritical Bulletin has been phased with calendar years starting with Bulletin 105 in 2016.

These meteorites are listed in the Meteoritical
Bulletin Database available online at [https://www.lpi](https://www.lpi.

usra.edu/meteor/. This database is widely used by meteorite scientists, meteorite educators and their students, and meteorite collectors. In 2024, the database has reached a daily total of between 5000 and 10,000 views of individual meteorite pages.

The meteorites listed in MB113 total 5660 kg of material. Twenty-two of these meteorites are reported to weigh over 50 kg, and 15 of those are ordinary chondrites (OCs). The non-OC meteorites with masses greater than 50 kg include Ramlat Fasad 555 (eucrite-melt breccia) with 365 kg, Saumalkol (ungrouped chondrite) with

<footnote n="1"><sup>1</sup>CNRS, Aix Marseille Univ, IRD, INRAE, CEREGE, Aix-en-Provence, France</footnote>

<footnote n="2"><sup>2</sup>NASA Johnson Space Center, Houston, Texas, USA</footnote>

<footnote n="3"><sup>3</sup>Reston, Virginia, USA</footnote>

<footnote n="4"><sup>4</sup>Buseck Center for Meteorite Studies, School of Earth and Space Exploration, Arizona State University, Tempe, Arizona, USA</footnote>

<footnote n="5"><sup>5</sup>Université de Lorraine, CNRS, CRPG, Nancy, France</footnote>

<footnote n="6"><sup>6</sup>Specola Vaticana, Vatican City State</footnote>

<footnote n="7"><sup>7</sup>Lunar and Planetary Institute, USRA-Houston, Houston, Texas, USA</footnote>

<footnote n="8"><sup>8</sup>Museum für Naturkunde, Leibniz-Institut für Biodiversitätsforschung, Berlin, Germany</footnote>

<footnote n="9"><sup>9</sup>Department of Earth and Planetary Sciences, Rutgers University, Piscataway, New Jersey, USA</footnote>

<footnote n="10"><sup>10</sup>Department of Earth and Environmental Sciences, The University of Manchester, Manchester, UK</footnote>

<footnote n="11"><sup>11</sup>Guilin University of Technology, Guilin, Guangxi Province, China</footnote>

<footnote n="12"><sup>12</sup>Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, Texas, USA</footnote>

<footnote n="13"><sup>13</sup>Astromaterials Research and Exploration Science (ARES) Division, XI3, NASA Johnson Space Center, Houston, Texas, USA</footnote>
163 kg, NWA 16525 (monomict eucrite) with 100 kg, NEA 051 (IIIAB iron) with 100 kg, NWA 16807 (IAB iron) with 71 kg, NWA 16760 (lunar melt breccia) with 62 kg, and Ksar Ghilane 022 (ungrouped achondrite) with 50 kg.

In detail, 1250 meteorites were collected in Antarctica (with over 90% from Asuka, Dominion Range, Elephant Moraine, Grove Mountains, and Yamato ice fields), 1102 in Africa, 689 in Asia, 575 in South America, 17 in North America, 11 in Europe, and 2 in Oceania (Figure 1). Like in MB112, it is noteworthy that 12% of North African meteorites now have geographic coordinates, and hence get a dense collection area name distinct from the typical Northwest Africa (NWA) or Northeast Africa (NEA) name. Another noteworthy feature is the increased number of meteorites recovered in the deserts of China (122), compared with previous years.

The meteorites listed in MB113 include 17 falls (11 ordinary chondrites, including an unequilibrated one, two EH3 chondrites, one CVox3, one CO3, one CM2, and one aubrite) that occurred in 2024 (4 falls), 2023 (5 falls), 2022 (2 falls), and 2021, 2018, 2012, 2007, 1994, and 1977 (1 fall each). Out of the 11 falls that occurred in 2022 or later, eight (73%) were recovered with the assistance of camera networks, such as the Desert Fireball Network in Australia (Bland et al., 2012), or international networks such as FRIPON (Colas et al., 2020), and/or radar reflectivity data (Fries & Fries, 2010). This record percentage highlights the increasing efficiency of these techniques, which likely

<figure><img src="image_2.png" /></figure>

FIGURE 2. Number of recovered meteorite falls per year since 2006 (open circles). The numbers for 2022 and 2023 are likely slightly underestimated due to the possible lag in declaring meteorite finds from new falls. The broken line is a linear fit (slope 0.26 fall/year). The gray bars are the percentage of falls that were recovered with the help of camera networks or weather radar imagery.

contribute to a steady increase in meteorite fall recovery over the last 15 years (Figure 2). In some countries (Australia, Czech Republic, Germany, and USA), close to 100% of the recovered falls have been found using strewnfield predictions from camera networks or weather radar systems.

The meteorites listed in MB113 comprise 2964 ordinary chondrites, 218 HED, 158 carbonaceous chondrites (including 7 ungrouped), 59 lunar meteorites (for a combined total of 243 kg of new material), 38 iron meteorites (9 ungrouped), 30 ureilites, 31 primitive achondrites (3 ungrouped), 28 mesosiderites, 24 enstatite chondrites, 21 martian meteorites (for a combined total of 30 kg of material), 24 ungrouped stony achondrites, 20 Rumuruti chondrites, 17 pallasites, 8 angrites, 5 enstatite achondrites (one ungrouped), and 1 ungrouped chondrite.

An unusually high number of meteorites (227) were reclassified in MB113. These are mostly CV chondrites that have been newly assigned to the CVox or CVred groups.

The following references were used to support the classification of meteorites in MB113: Barrat et al. (2003), Gardiol et al. (2020), Gattacceca et al. (2020), Giguere et al. (2000), Greenwood et al. (2005), Grossman and Brearley (2005), Hahn et al. (2018), Irving et al. (2022), Jarosewich (2006), King et al. (2021), Krämer Ruggiu et al. (2021), Macke et al. (2011), Maurel et al. (2024), Metzler (2012), Mittlefehldt et al. (2021), Neal and

<figure><img src="image_3.png" /></figure>

FIGURE 1. Number of meteorites from Antarctica, Northwest Africa, South America, and Asia reported in the last 11 Meteoritical Bulletins. These Meteoritical Bulletins are phased with civil years, starting with MB103 reporting meteorites approved by the Nomenclature Committee in 2014.
Taylor (1992), Pourkhorsandi et al. (2017), Pratesi et al. (2021), Rochette et al. (2003), Rochette et al. (2008), Rubin (2016), Rubin and Li (2019), Rubin and Ma (2019), Sharp and Wostbrock (2021), Sheikh (2021), Stoeffler et al. (1980), Torrano et al. (2020), Uehara and Gattacceca (2023), Vaci (2021), Vaci et al. (2021), Wasson and Kallemeyn (2002), Wasson and Choi (2003), Wasson and Huber (2006), Wasson et al. (1998), Wasson et al. (2007), Wilson et al. (2024), and Zurfluh et al. (2016).

## NOTABLE METEORITES

Oued Chebeika 002 (CI1, 418 g) is only the sixth CI1 chondrite, aside from the four Yamato chondrites that are either unrelated to CI chondrites or impact-dehydrated CI chondrites (Schrader et al., 2025; Zhu et al., 2025). Oued Chebeika 002 stands out among CI1 chondrites by the near absence of terrestrial alteration (Gattacceca et al., 2025). Together with Ryugu and Bennu samples (Connolly et al., 2025; Yokoyama et al., 2023), it provides a new source of pristine CI1 material. Saumalkol is a 163-kg ungrouped chondrite of petrological type 4. Ksar Ghilane 022 is a 50-kg ungrouped achondrite that has some geochemical affinities to aubrites but is composed predominantly of Fe-free augite rather than enstatite. NWA 16760 lunar melt breccia is the third largest lunar meteorite by mass. Three carbonaceous falls are listed in MB113: Ankazomena (only the 6th CVox3 fall), Boorama (only the 7th CO3 fall), and Shidian (CM2). This occurred only once before, in MB109 with Kolang (CM1/2), Flesnburg (C1-ung), and Tarda (C2-ung). NEA 071, a 2.36-kg CBb, is only the 26th CB chondrite and the 5th largest by mass.

In the impressive 17 observed falls that are included in MB113, Ribbeck (aubrite; fell January 21, 2024, Germany) is only the 12th aubrite fall and the third one since 2021 (Bischoff et al., 2024). Remarkably, two EH3 falls appear in MB113, Ait Saoun from Morocco (August 6, 2024) and Raja from Oman (December 23, 2023); which is also Oman's 2nd observed fall. This doubled the known number of EH3 falls (after Qingzhen from 1976 and Parsa from 1942). Takapō (L5; fell March 13, 2024) is the third observed fall in New Zealand's history, after Auckland (L5; fell 2004) and Mokoia (CV3; fell 1908). The US state of Arizona recorded its sixth observed meteorite fall with La Posa Plain (LL3-6). Charlottetown (H5) is the first-ever meteorite fall whose impact on the ground was recorded on video.

## ALPHABETICAL TEXT ENTRIES FOR NON-ANTARCTIC METEORITES

See the online version of this article.

## NEW DENSE COLLECTION AREAS

In 2022, 43 new dense collection areas (DCAs) were created: 17 in China, 9 in Algeria, 5 in Iran, 4 in Libya, 3 in Mali, 1 in Mauritania, 1 in Morocco, 1 in Peru, 1 in Tunisia, and 1 in Western Sahara. A full list of all approved DCAs, with maps, can be found at https://www.lpi.usra.edu/meteor/DenseAreas.php. New DCAs are named in collaboration with the following regional consultants: Djelloul Belhai (Algeria, Libya, Mali), Bingkui Miao (China), Elycheikh Naviee (Mauritania), Hasnaa Chennaoui (Morocco).

## LISTING OF INSTITUTES AND COLLECTIONS

An up-to-date index of collections and approved repositories (next to a green check mark) cited in the Meteorite Bulletin can be found here: https://www.lpi.usra.edu/meteor/MetBullAddresses.php?grp=country.

*Data Availability Statement*—The data that support the findings of this study are available in the supplementary material of this article.

*Editorial Handling*—Dr. A. J. Timothy Jull

## REFERENCES

Barrat, J. A., Jambon, A., Bohn, M., Blichert-Toft, J., Sautter, V., Göpel, C., Gillet, P., Boudouma, O., and Keller, F. 2003. Petrology and Geochemistry of the Unbrecciated Achondrite Northwest Africa 1240 (NWA 1240): An HED Parent Body Impact Melt. *Geochimica et Cosmochimica Acta* 67: 3959–70.

Bischoff, A. B., Bischoff, A., Patzek, M., Barrat, J.-. A., Berndt, J., Busemann, H., Degering, D., et al. 2024. Cosmic Pears from the Havelland (Germany): Ribbeck, the Twelfth Recorded Aubrite Fall in History. *Meteoritics & Planetary Science* 59: 2660–94.

Bland, P. A., Spurny, P., Bevan, A. W. R., Howard, K. T., Towner, M. C., Benedix, G. K., Greenwood, R. C., et al. 2012. The Australian Desert Fireball Network: A New Era for Planetary Science. *Australian Journal of Earth Sciences* 59: 177–187.

Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., et al. 2020. FRIPON: A Worldwide Network to Track Incoming Meteoroids. *Astronomy & Astrophysics* 644: A53.

Connolly, H. C., Lauretta, D. S., McCoy, T. J., Russell, S. S., Haenencour, P., Polit, A., Barnes, J. J., et al. 2025. An Overview of the Petrography and Petrology of Particles from Aggregate Sample from Asteroid Bennu. *Meteoritics & Planetary Science* 60: 979–996. https://doi.org/10.1111/maps.14335.

Fries, M., and Fries, J. 2010. Doppler Weather Radar as a Meteorite Recovery Tool. *Meteoritics & Planetary Science* 45: 1476–87.

Gardiol, D., Barghini, D., Buzzoni, A., Carbognani, A., di Carlo, M., di Martino, M., Knapic, C., et al. 2020.
Cavezzo, the First Italian Meteorite Recovered by the PRISMA Fireball Network. Orbit, Trajectory, and Strewn-Field. *Monthly Notices of the Royal Astronomical Society* 501: 1215-27.

Gattacceca, J., Bonal, L., Sonzogni, C., and Longerey, J. 2020. CV Chondrites: More than One Parent Body. *Earth and Planetary Science Letters* 547: 116467.

Gattacceca, J., Gounelle, M., Devouard, B., Barrat, J.-A., Bonal, L., King, A. J., Maurel, C., et al. 2025. Oued Chebea 002: A New C11 Meteorite Linked to Outer Solar System Bodies. *Meteoritics & Planetary Science*. https://doi.org/10.1111/MAPS.14359.

Giguere, T. A., Taylor, G. J., Hawke, B. R., and Lucey, P. G. 2000. The Titanium Contents of Lunar Mare Basalts. *Meteoritics & Planetary Science* 35: 193-200.

Greenwood, R. C., Franchi, I. A., Jambon, A., and Buchanan, P. C. 2005. Widespread Magma Oceans on Asteroidal Bodies in the Early Solar System. *Nature* 435: 916-128.

Grossman, J. N., and Brearley, A. J. 2005. The Onset of Metamorphism in Ordinary and Carbonaceous Chondrites. *Meteoritics & Planetary Science* 40: 87-122.

Hahn, T. M., Lunning, N. G., McSween, H. Y., Bodnar, R. J., and Taylor, L. A. 2018. Mg-Rich Harzburgites from Vesta: Mantle Residua or Cumulates from Planetary Differentiation? *Meteoritics & Planetary Science* 53: 514-546.

Irving, A. J., Gattacceca, J., Ziegler, K., Sonzogni, C., Carpenter, P. K., and Garvie, L. A. J. 2022. CT Chondrites: A Newly Recognized Carbonaceous Chondrite Group with Multiple Members, Including Telakoast 001, Chwichiya 002, and Cimarron. *53rd Lunar and Planetary Science Conference*. LPI Contribution No. 2678, 2022, abstract #2046.

Jarosewich, E. 2006. Chemical Analyses of Meteorites at the Smithsonian Institution: An Update. *Meteoritics & Planetary Science* 41: 1381-82.

King, A. J., Schofield, P. F., and Russell, S. S. 2021. Thermal Alteration of CM Carbonaceous Chondrites: Mineralogical Changes and Metamorphic Temperatures. *Geochimica et Cosmochimica Acta* 298: 167-190.

Krämer Ruggiu, L., Beck, P., Gattacceca, J., and Eschrig, J. 2021. Visible-Infrared Spectroscopy of Ungrouped and Rare Meteorites Brings Further Constraints on Meteorite-Asteroid Connections. *Icarus* 362: 114393.

Macke, R. J., Consolmagno, G. J., and Britt, D. T. 2011. Density, Porosity, and Magnetic Susceptibility of Carbonaceous Chondrites. *Meteoritics & Planetary Science* 46: 1842-62.

Maurel, C., Gattacceca, J., and Uehara, M. 2024. Hayabusa 2 Returned Samples Reveal a Weak to Null Magnetic Field during Aqueous Alteration of Ryugu's Parent Body. *Earth and Planetary Science Letters* 627: 118559.

Metzler, K. 2012. Ultrarapid Chondrite Formation by Hot Chondrule Accretion? Evidence from Unequilibrated Ordinary Chondrites. *Meteoritics & Planetary Science* 47: 2193-2217.

Mittlefehldt, D. W., Greenwood, R. C., Berger, E. L., Le, L., Peng, Z. X., and Ross, D. K. 2021. Eucrite-Type Achondrites: Petrology and Oxygen Isotope Compositions. *Meteoritics & Planetary Science* 57: 484-526.

Neal, C. R., and Taylor, L. A. 1992. Petrogenesis of Mare Basalts: A Record of Lunar Volcanism. *Geochimica et Cosmochimica Acta* 56: 2177-2211.

Pourkhorsandi, H., Gattacceca, J., Devouard, B., D'Orazio, M., Rochette, P., Beck, P., Sonzogni, C., and Valenzuela, M. 2017. The Ungrouped Chondrite El Médano 301 and its Comparison with Other Reduced Ordinary Chondrites. *Geochimica et Cosmochimica Acta* 218: 98-113.

Pratesi, G., Moggi Cecchi, V., Greenwood, R. C., Franchi, I. A., Hammond, S. J., Di Martino, M., Barghini, D., Taricco, C., Carbognani, A., and Gardiol, D. 2021. Cavezzo—The Double Face of a Meteorite: Mineralogy, Petrography, and Geochemistry of a Very Unusual Chondrite. *Meteoritics & Planetary Science* 56: 1125-50.

Rochette, P., Gattacceca, J., Bonal, L., Bourot-Denise, M., Chevrier, V., Clerc, J.-P., Consolmagno, G., et al. 2008. Magnetic Classification of Stony Meteorites: 2. Non-ordinary Chondrites. *Meteoritics & Planetary Science* 43: 959-980.

Rochette, P., Sagnotti, L., Bourot-Denise, M., Consolmagno, G., Folco, L., Gattacceca, J., Osete, M. L., and Pesonen, L. 2003. Magnetic Classification of Stony Meteorites: 1. Ordinary Chondrites. *Meteoritics & Planetary Science* 38: 251-268.

Rubin, A. E. 2016. Impact Melting of the Largest Known Enstatite Meteorite: Al Haggounia 001, a Fossil EL Chondrite. *Meteoritics & Planetary Science* 51: 1576-87.

Rubin, A. E., and Li, Y. 2019. Formation and Destruction of Magnetite in CO3 Chondrites and Other Chondrite Groups. *Geochemistry* 79: 125528.

Rubin, A. E., and Ma, C. 2019. Corrigendum to: "Meteoritic Minerals and their Origins" [Chemie der Erde—Geochemistry Volume 77, Issue September 2017, Pages 325-385]. *Geochemistry* 79: 189-198.

Schrader, D. L., Torrano, Z. A., Foustoukos, D. I., Alexander, C. M. O'D., Render, J., and Brennecka, G. A. 2025. Reassessing the Proposed "CY Chondrites": Evidence for Multiple Meteorite Types and Parent Bodies from Cr-Ti-H-C-N Isotopes and Bulk Elemental Compositions. *Geochimica et Cosmochimica Acta* 390: 24-37.

Sharp, Z. D., and Wostbrock, J. A. G. 2021. Standardization for the Triple Oxygen Isotope System: Waters, Silicates, Carbonates, Air, and Sulfates. *Reviews in Mineralogy and Geochemistry* 86: 179-196.

Sheikh, D. 2021. Petrology and Geochemistry of Errachidia 004, a Polymict Winonaite Composed of Distinct High and Low Metal Lithologies 84th Annual Meeting of the Meteoritical Society, August 15-21, 2021, Chicago, IL. LPI Contribution No. 2609, abstract 6253.

Stoeffler, D., Knoell, H.-D., Marvin, U. B., Simonds, C. H., and Warren, P. H. 1980. Recommended Classification and Nomenclature of Lunar Highland Rocks—A Committee Report. In *Conference on the Lunar Highlands Crust, Houston, Tex., November 14-16, 1979, Proceedings (A81-26201 10-91)*, 51-70. New York and Oxford: Pergamon Press.

Torrano, Z., Davidson, J., and Wadhwa, M. 2020. A Reclassification of Northwest Africa 2900 from CV3 to CK3 Chondrite. *Meteoritics & Planetary Science* 55: 2539-50.

Uehara, M., and Gattacceca, J. 2023. The "Meteorite Meter": A Handheld Instrument for the Combined Measurement of Magnetic Susceptibility and Electrical Conductivity, with Application to Meteorite Identification and Classification. *Meteoritics & Planetary Science* 58: 1629-41.

Vaci, Z. 2021. Petrology and Geochemistry of Evolved Achondrites: *Planetesimal Mantles and Crusts*. Albuquerque, New Mexico, USA: University of New Mexico Dissertation.

Vaci, Z., Ziegler, K., Yang, S., Humayun, M., and Agee, C. B. 2021. Northwest Africa 6698: Dioritic Partial Melt of
the Ureilite Parent Body. 52nd Lunar and Planetary
Science Conference (LPI Contrib. No. 2548).

Wasson, J. T., and Choi, B.-G. 2003. Main-Group Pallasites. *Geochimica et Cosmochimica Acta* 67: 3079–96.

Wasson, J. T., Choi, B.-G., Jerde, E. A., and Ulff-Møller, F. 1998. Chemical Classification of Iron Meteorites: XII. New Members of the Magmatic Groups. *Geochimica et Cosmochimica Acta* 62: 715–724.

Wasson, J. T., and Huber, H. 2006. Compositional Trends among IID Irons; their Possible Formation from the P-Rich Lower Magma in a Two-Layer Core. *Geochimica et Cosmochimica Acta* 70: 6153–67.

Wasson, J. T., Huber, H., and Malvin, D. J. 2007. Formation of IIAB Iron Meteorites. *Geochimica et Cosmochimica Acta* 71: 760–781.

Wasson, J. T., and Kallemeyn, G. W. 2002. The IAB Iron-Meteorite Complex: A Group, Five Subgroups, Numerous Grouplets, Closely Related, Mainly Formed by Crystal Segregation in Rapidly Cooling Melts. *Geochimica et Cosmochimica Acta* 66: 2445–73.

SUPPORTING INFORMATION

Additional supporting information may be found in
the online version of this article.

**Table S1.** Meteorite Bulletin No. 113 data including
Antarctic meteorites.

Wilson, B. J. K., Di Cecco, V. E., Garvie, L. A. J., Tait, K. T., and Daly, M. G. 2024. A Sample Preparation Guide for Clay-Rich Carbonaceous Chondrites. *Meteoritics & Planetary Science* 59: 560–67.

Yokoyama, T., Nagashima, K., Nakai, I., Young, E. D., Abe, Y., Aléon, J., Alexander, C. M. O.'. D., et al. 2023. Samples Returned from the Asteroid Ryugu Are Similar to Ivuna-Type Carbonaceous Meteorites. *Science* 379: eabn7850.

Zhu, K., Nakanishi, N., Render, J., Shollenberg, Q. R., Yokoyama, T., Ishikawa, A., and Chen, L. 2025. CY1 Chondrites Produced by Impact-Dehydration of the CI Chondrite Parent Body? *Astrophysical Journal Letters* 987:L54. https://doi.org/10.3847/2041-8213/adc89c

Zurfluh, F. J., Hofmann, B. A., Gnos, E., Eggenberger, U., and Jull, A. J. T. 2016. Weathering of Ordinary Chondrites from Oman: Correlation of Weathering Parameters with 14C Terrestrial Ages and a Refined Weathering Scale. *Meteoritics & Planetary Science* 51: 1685–1700.

**Table S2.** Corrections to the Meteoritical Bulletin
Database.

**Data S1.** Writeups from MetBull 113.