Dataset Information

Metals from spacecraft reentry in stratospheric aerosol particles.

ABSTRACT: Large increases in the number of low earth orbit satellites are projected in the coming decades [L. Schulz, K.-H. Glassmeier, Adv. Space Res. 67, 1002-1025 (2021)] with perhaps 50,000 additional satellites in orbit by 2030 [GAO, Large constellations of satellites: Mitigating environmental and other effects (2022)]. When spent rocket bodies and defunct satellites reenter the atmosphere, they produce metal vapors that condense into aerosol particles that descend into the stratosphere. So far, models of spacecraft reentry have focused on understanding the hazard presented by objects that survive to the surface rather than on the fate of the metals that vaporize. Here, we show that metals that vaporized during spacecraft reentries can be clearly measured in stratospheric sulfuric acid particles. Over 20 elements from reentry were detected and were present in ratios consistent with alloys used in spacecraft. The mass of lithium, aluminum, copper, and lead from the reentry of spacecraft was found to exceed the cosmic dust influx of those metals. About 10% of stratospheric sulfuric acid particles larger than 120 nm in diameter contain aluminum and other elements from spacecraft reentry. Planned increases in the number of low earth orbit satellites within the next few decades could cause up to half of stratospheric sulfuric acid particles to contain metals from reentry. The influence of this level of metallic content on the properties of stratospheric aerosol is unknown.

SUBMITTER: Murphy DM

PROVIDER: S-EPMC10614211 | biostudies-literature | 2023 Oct

REPOSITORIES: biostudies-literature

ACCESS DATA

Publications

Metals from spacecraft reentry in stratospheric aerosol particles.

Murphy Daniel M DM Abou-Ghanem Maya M Cziczo Daniel J DJ Froyd Karl D KD Jacquot Justin J Lawler Michael J MJ Maloney Christopher C Plane John M C JMC Ross Martin N MN Schill Gregory P GP Shen Xiaoli X

Proceedings of the National Academy of Sciences of the United States of America 20231016 43

Large increases in the number of low earth orbit satellites are projected in the coming decades [L. Schulz, K.-H. Glassmeier, <i>Adv. Space Res.</i> <b>67</b>, 1002-1025 (2021)] with perhaps 50,000 additional satellites in orbit by 2030 [GAO, Large constellations of satellites: Mitigating environmental and other effects (2022)]. When spent rocket bodies and defunct satellites reenter the atmosphere, they produce metal vapors that condense into aerosol particles that descend into the stratosphere ...[more]

PMID: 37844220

Similar Datasets

Project description:The Ozone Mapping and Profiler Suite Limb Profiler (OMPS/LP) has been flying on the Suomi NPP satellite since October 2011. It is designed to produce ozone and aerosol vertical profiles at ~2 km vertical resolution over the entire sunlit globe. Aerosol extinction profiles are computed with Mie theory using radiances measured at 675 nm. The operational Version 1.0 (V1.0) aerosol extinction retrieval algorithm assumes a bimodal lognormal aerosol size distribution (ASD) whose parameters were derived by combining an in situ measurement of aerosol microphysics with the SAGE II aerosol extinction climatology. Internal analysis indicates that this bimodal lognormal ASD does not sufficiently explain the spectral dependence of LP measured radiances. In this paper we describe the derivation of an improved aerosol size distribution, designated Version 1.5 (V1.5), for the LP retrieval algorithm. The new ASD uses a gamma function distribution that is derived from Community Aerosol and Radiation Model for Atmospheres (CARMA) calculated results. A cumulative distribution fit derived from the gamma function ASD gives better agreement with CARMA results at small particle radii than bimodal or unimodal functions. The new ASD also explains the spectral dependence of LP measured radiances better than the V1.0 ASD. We find that the impact of our choice of ASD on the retrieved extinctions varies strongly with the underlying reflectivity of the scene. Initial comparisons with co-located extinction profiles retrieved at 676 nm from the SAGE III/ISS instrument show a significant improvement in agreement for the LP V1.5 retrievals. Zonal mean extinction profiles agree to within 10% between 19-29 km, and regression fits of collocated samples show improved correlation and reduced scatter compared to the V1.0 product. This improved agreement will motivate development of more sophisticated ASDs from CARMA results that incorporate latitude, altitude, and seasonal variations in aerosol properties.

Project description:NASA cleanrooms are certified by particle counts and are humidity-controlled, temperature-regulated, and oligotrophic in nature for assembling spacecraft subsystems. Microorganisms, which are not part of the cleanroom certification metrics, should not be overlooked when assessing the cleanliness of the facility since they can enter through soil or air, shed from humans, adapt to the oligotrophic conditions, and subsequently could contaminate spacecraft. These biogenic particles need to be identified to extend our knowledge of biological contamination for future NASA mission use. This study collected particles from the cleanroom and estimated the distribution of fallout microbial cell and inert dust particles using microscopy and molecular techniques. Aluminum coupon-based polycarbonate filter assemblies were deployed in the spacecraft assembly cleanroom facility to collect fallout particles. Epifluorescence and electron microscopy showed that particles varied in size and structure, and displayed live/dead biological and inert particle signatures from sources that include spores and fungal hyphae. Additionally, correlative epifluorescence and field emission scanning electron microscopy, combined with energy-dispersive X-ray analysis (for elemental compositions) methods, differentiated whether microbes adhering to particles were live/dead cells or inert particles. This visualization approach allowed for the classification of microorganisms as being standalone (free-living) or associated with a particle, as well as its characteristic size. Furthermore, time-course microscopy was used to determine the microbial cell growth and confirm the biological/molecular identification. Routine investigation of cleanroom biological and inert fallout particles will help to determine the biological load of spacecraft components and will also have direct relevance to the pharmaceutical and medical industries. One of the main objectives for NASA's current and future missions is to prevent forward and back contamination of exploring planets. The goal of this study is to determine the association of microorganisms with the inert, natural cleanroom fallout particles and to ascertain whether microorganisms prefer to adhere to a particle size. A novel microscopy technique was developed, and by utilizing various molecular techniques, particles and associated microbial phylogeny were characterized. An accurate assessment of the microbes associated with cleanroom particles is necessary to protect the health of the people who occupy the room for long duration for aeronautical, medical, and pharmaceutical industries.

Dataset Information

Metals from spacecraft reentry in stratospheric aerosol particles.

Publications

Metals from spacecraft reentry in stratospheric aerosol particles.

Similar Datasets

OmicsDI is part of the ELIXIR infrastructure

Tweets