Comet Formation in the Framework of Streaming Instability Article Swipe
Sebastian Lorek
·
YOU?
·
· 2018
· Open Access
·
· DOI: https://doi.org/10.24355/dbbs.084-201811010920-0
YOU?
·
· 2018
· Open Access
·
· DOI: https://doi.org/10.24355/dbbs.084-201811010920-0
The bodies of the solar system formed 4.6 Gyr ago in the protoplanetary disk around the young protosun. Starting with submicrometre-sized dust and ice grains, collisions and coalescence led to the formation of aggregates, planetesimals, and eventually planets. Comets are believed to be the kilometre-sized icy planetesimals that were not accreted into larger bodies and have survived until today. It is poorly understood how bodies manage to grow to sizes larger than about millimetre to decimetre because bouncing and fragmentation terminate growth well below kilometres. Streaming instability arising from the coupling between the gas and millimetre- to decimetre-sized dust aggregates via drag is a promising mechanism to bridge this gap. The instability produces locally high dust densities which collapse due to self-gravity and form planetesimals in the size range kilometres to a few hundred kilometres. Planetesimal formation through streaming instability predicts objects with characteristic properties of comets. This thesis investigates the formation of comets in the framework of the streaming instability. Aggregate growth in the solar nebula is modelled to find the specific properties of the aggregates that eventually trigger the streaming instability. Simulations of the gravitational collapse of a cloud of porous aggregates (pebble cloud) are conducted to address the questions how aggregate properties change during the collapse and whether or not the resulting planetesimal has the properties of a comet.
Related Topics
Concepts
Planetesimal
Formation and evolution of the Solar System
Streaming instability
Astrobiology
Instability
Physics
Solar System
Gravitational collapse
Gravitational instability
Comet
Coalescence (physics)
Millimeter
Fragmentation (computing)
Protoplanet
Astronomy
Geology
Mechanics
Operating system
Computer science
Metadata
- Type
- dissertation
- Language
- en
- Landing Page
- http://uri.gbv.de/document/gvk:ppn:1042363978
- https://nbn-resolving.org/urn:nbn:de:gbv:084-2018110109213
- OA Status
- green
- References
- 8
- Related Works
- 19
- OpenAlex ID
- https://openalex.org/W2955685111
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2955685111Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.24355/dbbs.084-201811010920-0Digital Object Identifier
- Title
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Comet Formation in the Framework of Streaming InstabilityWork title
- Type
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dissertationOpenAlex work type
- Language
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enPrimary language
- Publication year
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2018Year of publication
- Publication date
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2018-11-01Full publication date if available
- Authors
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Sebastian LorekList of authors in order
- Landing page
-
https://uri.gbv.de/document/gvk:ppn:1042363978Publisher landing page
- PDF URL
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https://nbn-resolving.org/urn:nbn:de:gbv:084-2018110109213Direct link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
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https://nbn-resolving.org/urn:nbn:de:gbv:084-2018110109213Direct OA link when available
- Concepts
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Planetesimal, Formation and evolution of the Solar System, Streaming instability, Astrobiology, Instability, Physics, Solar System, Gravitational collapse, Gravitational instability, Comet, Coalescence (physics), Millimeter, Fragmentation (computing), Protoplanet, Astronomy, Geology, Mechanics, Operating system, Computer scienceTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
0Total citation count in OpenAlex
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8Number of works referenced by this work
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19Other works algorithmically related by OpenAlex
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| abstract_inverted_index.were | 48 |
| abstract_inverted_index.with | 19, 142 |
| abstract_inverted_index.about | 72 |
| abstract_inverted_index.below | 83 |
| abstract_inverted_index.cloud | 190 |
| abstract_inverted_index.range | 128 |
| abstract_inverted_index.sizes | 69 |
| abstract_inverted_index.solar | 4, 165 |
| abstract_inverted_index.until | 57 |
| abstract_inverted_index.which | 117 |
| abstract_inverted_index.young | 16 |
| abstract_inverted_index.Comets | 38 |
| abstract_inverted_index.around | 14 |
| abstract_inverted_index.bodies | 1, 53, 64 |
| abstract_inverted_index.bridge | 107 |
| abstract_inverted_index.change | 205 |
| abstract_inverted_index.cloud) | 195 |
| abstract_inverted_index.comet. | 221 |
| abstract_inverted_index.comets | 153 |
| abstract_inverted_index.during | 206 |
| abstract_inverted_index.formed | 6 |
| abstract_inverted_index.growth | 81, 162 |
| abstract_inverted_index.larger | 52, 70 |
| abstract_inverted_index.manage | 65 |
| abstract_inverted_index.nebula | 166 |
| abstract_inverted_index.poorly | 61 |
| abstract_inverted_index.porous | 192 |
| abstract_inverted_index.system | 5 |
| abstract_inverted_index.thesis | 148 |
| abstract_inverted_index.today. | 58 |
| abstract_inverted_index.(pebble | 194 |
| abstract_inverted_index.address | 199 |
| abstract_inverted_index.arising | 87 |
| abstract_inverted_index.because | 76 |
| abstract_inverted_index.between | 91 |
| abstract_inverted_index.comets. | 146 |
| abstract_inverted_index.grains, | 24 |
| abstract_inverted_index.hundred | 133 |
| abstract_inverted_index.locally | 113 |
| abstract_inverted_index.objects | 141 |
| abstract_inverted_index.through | 137 |
| abstract_inverted_index.trigger | 179 |
| abstract_inverted_index.whether | 210 |
| abstract_inverted_index.Starting | 18 |
| abstract_inverted_index.accreted | 50 |
| abstract_inverted_index.believed | 40 |
| abstract_inverted_index.bouncing | 77 |
| abstract_inverted_index.collapse | 118, 187, 208 |
| abstract_inverted_index.coupling | 90 |
| abstract_inverted_index.modelled | 168 |
| abstract_inverted_index.planets. | 37 |
| abstract_inverted_index.predicts | 140 |
| abstract_inverted_index.produces | 112 |
| abstract_inverted_index.specific | 172 |
| abstract_inverted_index.survived | 56 |
| abstract_inverted_index.Aggregate | 161 |
| abstract_inverted_index.Streaming | 85 |
| abstract_inverted_index.aggregate | 203 |
| abstract_inverted_index.conducted | 197 |
| abstract_inverted_index.decimetre | 75 |
| abstract_inverted_index.densities | 116 |
| abstract_inverted_index.formation | 31, 136, 151 |
| abstract_inverted_index.framework | 156 |
| abstract_inverted_index.mechanism | 105 |
| abstract_inverted_index.promising | 104 |
| abstract_inverted_index.protosun. | 17 |
| abstract_inverted_index.questions | 201 |
| abstract_inverted_index.resulting | 214 |
| abstract_inverted_index.streaming | 138, 159, 181 |
| abstract_inverted_index.terminate | 80 |
| abstract_inverted_index.aggregates | 99, 176, 193 |
| abstract_inverted_index.collisions | 25 |
| abstract_inverted_index.eventually | 36, 178 |
| abstract_inverted_index.kilometres | 129 |
| abstract_inverted_index.millimetre | 73 |
| abstract_inverted_index.properties | 144, 173, 204, 218 |
| abstract_inverted_index.understood | 62 |
| abstract_inverted_index.Simulations | 183 |
| abstract_inverted_index.aggregates, | 33 |
| abstract_inverted_index.coalescence | 27 |
| abstract_inverted_index.instability | 86, 111, 139 |
| abstract_inverted_index.kilometres. | 84, 134 |
| abstract_inverted_index.millimetre- | 95 |
| abstract_inverted_index.Planetesimal | 135 |
| abstract_inverted_index.instability. | 160, 182 |
| abstract_inverted_index.investigates | 149 |
| abstract_inverted_index.planetesimal | 215 |
| abstract_inverted_index.self-gravity | 121 |
| abstract_inverted_index.fragmentation | 79 |
| abstract_inverted_index.gravitational | 186 |
| abstract_inverted_index.planetesimals | 46, 124 |
| abstract_inverted_index.characteristic | 143 |
| abstract_inverted_index.planetesimals, | 34 |
| abstract_inverted_index.protoplanetary | 12 |
| abstract_inverted_index.decimetre-sized | 97 |
| abstract_inverted_index.kilometre-sized | 44 |
| abstract_inverted_index.submicrometre-sized | 20 |
| cited_by_percentile_year | |
| corresponding_author_ids | https://openalex.org/A5004941062 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 1 |
| citation_normalized_percentile.value | 0.13171882 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |