Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time
Abstract One of the outstanding questions in planetary science is to determine how the fundamental mechanical and physical properties of materials determine the thermal evolution of asteroids, and which properties have the greatest influence. We investigate the effects of uncertainty in the material...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2023-01-01
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| Series: | Earth, Planets and Space |
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| Online Access: | https://doi.org/10.1186/s40623-022-01751-x |
| _version_ | 1797946012088664064 |
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| author | Jonas Hallstrom Maitrayee Bose |
| author_facet | Jonas Hallstrom Maitrayee Bose |
| author_sort | Jonas Hallstrom |
| collection | DOAJ |
| description | Abstract One of the outstanding questions in planetary science is to determine how the fundamental mechanical and physical properties of materials determine the thermal evolution of asteroids, and which properties have the greatest influence. We investigate the effects of uncertainty in the material properties of asteroid parent bodies on the ability of thermal evolution models to constrain the sizes and formation times of ordinary chondrite parent asteroids. A simple model is formulated for the thermal evolution of the parent body of asteroid 25143 Itokawa. The effects of the uncertainties in the values specified for specific heat capacity, thermal diffusivity, and aluminum abundance are determined. The uncertainties in specific heat capacity and aluminum abundance, or heat production more generally, are found to both have significant and approximately equal effects on these results, substantially widening the range of possible formation times of Itokawa’s parent body. We show that Itokawa’s parent body could have formed between 1.6 and 2.5 million years after the origin of calcium–aluminum inclusions with a radius larger than 19 km, and it could have formed as early as 1.4 millions years, as late as 3.5 million years, or with a radius as small at 17 km if more lenient definitions of uncertainty in aluminum abundance are considered. These results stress the importance of precise data required of the material properties of a suite of LL type 4-6 ordinary chondrite meteorites to place better constraints on the thermal history of Itokawa’s parent body. Graphical Abstract |
| first_indexed | 2024-04-10T21:04:09Z |
| format | Article |
| id | doaj.art-5094b10aae2842f7993edc5fd9986a0d |
| institution | Directory Open Access Journal |
| issn | 1880-5981 |
| language | English |
| last_indexed | 2024-04-10T21:04:09Z |
| publishDate | 2023-01-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | Earth, Planets and Space |
| spelling | doaj.art-5094b10aae2842f7993edc5fd9986a0d2023-01-22T12:06:50ZengSpringerOpenEarth, Planets and Space1880-59812023-01-0175111310.1186/s40623-022-01751-xUncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation timeJonas Hallstrom0Maitrayee Bose1Department of Physics, Arizona State UniversitySchool of Earth and Space Exploration, Arizona State UniversityAbstract One of the outstanding questions in planetary science is to determine how the fundamental mechanical and physical properties of materials determine the thermal evolution of asteroids, and which properties have the greatest influence. We investigate the effects of uncertainty in the material properties of asteroid parent bodies on the ability of thermal evolution models to constrain the sizes and formation times of ordinary chondrite parent asteroids. A simple model is formulated for the thermal evolution of the parent body of asteroid 25143 Itokawa. The effects of the uncertainties in the values specified for specific heat capacity, thermal diffusivity, and aluminum abundance are determined. The uncertainties in specific heat capacity and aluminum abundance, or heat production more generally, are found to both have significant and approximately equal effects on these results, substantially widening the range of possible formation times of Itokawa’s parent body. We show that Itokawa’s parent body could have formed between 1.6 and 2.5 million years after the origin of calcium–aluminum inclusions with a radius larger than 19 km, and it could have formed as early as 1.4 millions years, as late as 3.5 million years, or with a radius as small at 17 km if more lenient definitions of uncertainty in aluminum abundance are considered. These results stress the importance of precise data required of the material properties of a suite of LL type 4-6 ordinary chondrite meteorites to place better constraints on the thermal history of Itokawa’s parent body. Graphical Abstracthttps://doi.org/10.1186/s40623-022-01751-xThermal evolution modelsItokawaChondritesAsteroids |
| spellingShingle | Jonas Hallstrom Maitrayee Bose Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time Earth, Planets and Space Thermal evolution models Itokawa Chondrites Asteroids |
| title | Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time |
| title_full | Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time |
| title_fullStr | Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time |
| title_full_unstemmed | Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time |
| title_short | Uncertainties in physical properties of Itokawa-like asteroids widen constraints on their formation time |
| title_sort | uncertainties in physical properties of itokawa like asteroids widen constraints on their formation time |
| topic | Thermal evolution models Itokawa Chondrites Asteroids |
| url | https://doi.org/10.1186/s40623-022-01751-x |
| work_keys_str_mv | AT jonashallstrom uncertaintiesinphysicalpropertiesofitokawalikeasteroidswidenconstraintsontheirformationtime AT maitrayeebose uncertaintiesinphysicalpropertiesofitokawalikeasteroidswidenconstraintsontheirformationtime |