dc.contributor.author
Suttle, M. D.
dc.contributor.author
Hasse, T.
dc.contributor.author
Hecht, Lutz
dc.date.accessioned
2021-09-08T08:05:23Z
dc.date.available
2021-09-08T08:05:23Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/31880
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-31612
dc.description.abstract
We report the recovery and characterization of a new urban micrometeorite collection derived from the rooftop of an industrial building in Germany. We identified 315 micrometeorites (diameter: 55–515 µm, size peak: ˜150 µm, size distribution slope exponent: −2.62). They are predominantly S-type cosmic spherules (97.2%) but also two G-type spherules (0.6%), an unmelted coarse-grained single-mineral micrometeorite, and eight scoriaceous particles (2.5%) or particles transitional between scoriaceous micrometeorites and porphyritic spherules. Their analysis details how the magnetite rim on partially melted micrometeorites is progressively diluted as the melt fraction increases during heating. At least 10 micrometeorites contain platinum group nuggets (PGNs). They have chondritic compositions but are depleted in volatile Pd. However, a single nugget preserves chondritic Pd concentrations. We suggest that an Fe-Ni-S bead originally containing the PGN escaped its host cavity and wet the particle exterior, creating an Fe-rich melt that protected the nugget from evaporation. This melt layer oxidized forming magnetite—indicating that wetting events can affect the texture and composition of micrometeorites. Utilizing the well-constrained surface area (8400 m2) and rooftop age (21 yr), we attempted the first global mass flux estimate based on urban micrometeorite data. This produced anomalously low values (13.4 t yr–1), even when correcting for losses due to sample processing (<89.7 t yr–1). Our value is approximately two orders of magnitude lower than previous estimates, indicating that >99% of particles are missing, having been lost via drainage and cleaning. Rooftop collection sites have limited potential for mass flux calculations unless problems of loss can be resolved. However, urban micrometeorite collections have other advantages, notably exceptionally well-preserved particles with extremely young terrestrial ages and the ability to extract many micrometeorites from accessible sites. Urban micrometeorites should be considered complementary to Antarctic and deep-sea collections with potential for citizen science and educational exploitation.
en
dc.format.extent
25 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by-nc/4.0/
dc.subject
urban micrometeorites
en
dc.subject
rooftop collection sites
en
dc.subject
urban micrometeorite collections
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
dc.title
Evaluating urban micrometeorites as a research resource—A large population collected from a single rooftop
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.doi
10.1111/maps.13712
dcterms.bibliographicCitation.journaltitle
Meteoritics & Planetary Science
dcterms.bibliographicCitation.number
8
dcterms.bibliographicCitation.pagestart
1531
dcterms.bibliographicCitation.pageend
1555
dcterms.bibliographicCitation.volume
56
dcterms.bibliographicCitation.url
https://doi.org/10.1111/maps.13712
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Geochemie, Hydrogeologie, Mineralogie
refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1945-5100
refubium.resourceType.provider
WoS-Alert