Habitat Bennu: Design Concepts for Spinning Habitats Constructed From Rubble Pile Near-Earth Asteroids

The authors explore the possibility that near-earth, rubble pile asteroids might be used as habitats for human settlement by increasing their rotation to produce spin gravity. Using previously published scaling by Maindl et al. and studies of asteroid populations, it is shown that there is no class...

Full description

Saved in:
Bibliographic Details
Published inFrontiers in astronomy and space sciences Vol. 8
Main Authors Miklavčič, Peter M., Siu, John, Wright, Esteban, Debrecht, Alex, Askari, Hesam, Quillen, Alice C., Frank, Adam
Format Journal Article
LanguageEnglish
Published Frontiers Media S.A 03.01.2022
Subjects
Online AccessGet full text

Cover

Loading…
Abstract The authors explore the possibility that near-earth, rubble pile asteroids might be used as habitats for human settlement by increasing their rotation to produce spin gravity. Using previously published scaling by Maindl et al. and studies of asteroid populations, it is shown that there is no class of hollowed body that would survive the spin-up process on its own without additional reinforcement. Large solid-rock asteroids (diameter D > 10 km) would not have the tensile strength to withstand the required rotation rates and would fracture and break apart. Smaller asteroids, being ‘rubble piles’, have little tensile strength and would quickly disperse. The possibility of containing the asteroid mass using higher-strength materials like carbon nanofiber is instead considered. It is found that a moderate tensile strength container can maintain the integrity of a large spinning cylinder composed of dispersed asteroid regolith. The research extends the range of possible asteroid habitat candidates, since it may become feasible to construct habitats from the more numerous smaller bodies, including NEAs (Near Earth Asteroids). The required tensile strength of the container material scales with habitat radius and thickness and is ∼ 200 MPa for a starting asteroid body of radius 300 m that is spun up to provide 0.3  g ⊕ while increasing its radius to 3 km and maintaining a rubble and regolith shield thickness of 2 m to protect against cosmic rays. Ambient solar power can be harvested to aid in spin-up and material processing.
AbstractList The authors explore the possibility that near-earth, rubble pile asteroids might be used as habitats for human settlement by increasing their rotation to produce spin gravity. Using previously published scaling by Maindl et al. and studies of asteroid populations, it is shown that there is no class of hollowed body that would survive the spin-up process on its own without additional reinforcement. Large solid-rock asteroids (diameter D > 10 km) would not have the tensile strength to withstand the required rotation rates and would fracture and break apart. Smaller asteroids, being ‘rubble piles’, have little tensile strength and would quickly disperse. The possibility of containing the asteroid mass using higher-strength materials like carbon nanofiber is instead considered. It is found that a moderate tensile strength container can maintain the integrity of a large spinning cylinder composed of dispersed asteroid regolith. The research extends the range of possible asteroid habitat candidates, since it may become feasible to construct habitats from the more numerous smaller bodies, including NEAs (Near Earth Asteroids). The required tensile strength of the container material scales with habitat radius and thickness and is ∼ 200 MPa for a starting asteroid body of radius 300 m that is spun up to provide 0.3  g ⊕ while increasing its radius to 3 km and maintaining a rubble and regolith shield thickness of 2 m to protect against cosmic rays. Ambient solar power can be harvested to aid in spin-up and material processing.
The authors explore the possibility that near-earth, rubble pile asteroids might be used as habitats for human settlement by increasing their rotation to produce spin gravity. Using previously published scaling by Maindl et al. and studies of asteroid populations, it is shown that there is no class of hollowed body that would survive the spin-up process on its own without additional reinforcement. Large solid-rock asteroids (diameter D > 10 km) would not have the tensile strength to withstand the required rotation rates and would fracture and break apart. Smaller asteroids, being ‘rubble piles’, have little tensile strength and would quickly disperse. The possibility of containing the asteroid mass using higher-strength materials like carbon nanofiber is instead considered. It is found that a moderate tensile strength container can maintain the integrity of a large spinning cylinder composed of dispersed asteroid regolith. The research extends the range of possible asteroid habitat candidates, since it may become feasible to construct habitats from the more numerous smaller bodies, including NEAs (Near Earth Asteroids). The required tensile strength of the container material scales with habitat radius and thickness and is ∼ 200 MPa for a starting asteroid body of radius 300 m that is spun up to provide 0.3 g⊕ while increasing its radius to 3 km and maintaining a rubble and regolith shield thickness of 2 m to protect against cosmic rays. Ambient solar power can be harvested to aid in spin-up and material processing.
Author Siu, John
Debrecht, Alex
Miklavčič, Peter M.
Wright, Esteban
Quillen, Alice C.
Askari, Hesam
Frank, Adam
Author_xml – sequence: 1
  givenname: Peter M.
  surname: Miklavčič
  fullname: Miklavčič, Peter M.
– sequence: 2
  givenname: John
  surname: Siu
  fullname: Siu, John
– sequence: 3
  givenname: Esteban
  surname: Wright
  fullname: Wright, Esteban
– sequence: 4
  givenname: Alex
  surname: Debrecht
  fullname: Debrecht, Alex
– sequence: 5
  givenname: Hesam
  surname: Askari
  fullname: Askari, Hesam
– sequence: 6
  givenname: Alice C.
  surname: Quillen
  fullname: Quillen, Alice C.
– sequence: 7
  givenname: Adam
  surname: Frank
  fullname: Frank, Adam
BookMark eNpNkM1KAzEQgIMoqLUP4C0vsHWyyWaz3rRaK4iKP-AtJJtJjdSkJNuDb29rRbzMDDPDN8N3TPZjikjIKYMJ56o782VlyqSGmk2kaLjke-SorjtZdap92_9XH5JxKR8AwFSrOsmPiJ8bGwYz0EuMcX1Or7CERaTTFHtcDYX6lOnzKsQY4oL-7pbtuAx53Q_o6CynT_q0tnaJ9DFswj2aXF2bPLzTizJgTsGVE3LgzbLg-DePyOvs-mU6r-4ebm6nF3dVz0EOFetNJ7hUovbemEZIr-raocXWtaYWjgFwAI-KO9lYDsyAdVwCyka1Dhwfkdsd1yXzoVc5fJr8pZMJ-qeR8kJvHgv9ErV1gE4I1jsrRcutbQz24IXlykq1OTEibMfqcyolo__jMdBb7_rHu9561zvv_Bt1cnoJ
Cites_doi 10.1016/j.icarus.2005.04.001
10.1038/nature13632
10.1006/icar.1997.5776
10.1016/0019-1035(75)90035-4
10.1089/space.2016.0027
10.1126/science.aaw0422
10.1029/2019je006246
10.1371/journal.pone.0106207
10.3389/fspas.2019.00037
10.1006/icar.2000.6482
10.1146/annurev-astro-081817-052013
10.1007/978-3-662-45052-9_8
10.1016/j.bone.2008.11.014
10.1063/1.3128863
10.3357/asem.3520.2013
10.1155/2014/782390
10.1016/j.icarus.2010.07.009
10.1038/s41586-019-1033-6
10.1126/sciadv.abd3649
10.1016/j.asr.2014.08.019
10.1126/science.1126272
10.1096/fj.13-229195
10.1016/j.icarus.2019.113443
10.1063/pt.3.4438
10.1038/s41561-019-0326-6
ContentType Journal Article
DBID AAYXX
CITATION
DOA
DOI 10.3389/fspas.2021.645363
DatabaseName CrossRef
DOAJ Directory of Open Access Journals
DatabaseTitle CrossRef
DatabaseTitleList CrossRef

Database_xml – sequence: 1
  dbid: DOA
  name: DOAJ Directory of Open Access Journals
  url: https://www.doaj.org/
  sourceTypes: Open Website
DeliveryMethod fulltext_linktorsrc
Discipline Astronomy & Astrophysics
EISSN 2296-987X
ExternalDocumentID oai_doaj_org_article_bd0ed441cdb6473bb5aec0f4b38b68e8
10_3389_fspas_2021_645363
GroupedDBID 5VS
9T4
AAFWJ
AAYXX
ACGFS
ACXDI
ADBBV
AFPKN
ALMA_UNASSIGNED_HOLDINGS
BCNDV
CITATION
GROUPED_DOAJ
KQ8
M~E
OK1
ID FETCH-LOGICAL-c306t-1ca9436842ffaa546f822debe7d7a24d100300fe83d65b301a0bd360e6587d0d3
IEDL.DBID DOA
ISSN 2296-987X
IngestDate Wed Aug 27 01:29:26 EDT 2025
Tue Jul 01 02:58:43 EDT 2025
IsDoiOpenAccess true
IsOpenAccess true
IsPeerReviewed true
IsScholarly true
Language English
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c306t-1ca9436842ffaa546f822debe7d7a24d100300fe83d65b301a0bd360e6587d0d3
OpenAccessLink https://doaj.org/article/bd0ed441cdb6473bb5aec0f4b38b68e8
ParticipantIDs doaj_primary_oai_doaj_org_article_bd0ed441cdb6473bb5aec0f4b38b68e8
crossref_primary_10_3389_fspas_2021_645363
ProviderPackageCode CITATION
AAYXX
PublicationCentury 2000
PublicationDate 2022-01-03
PublicationDateYYYYMMDD 2022-01-03
PublicationDate_xml – month: 01
  year: 2022
  text: 2022-01-03
  day: 03
PublicationDecade 2020
PublicationTitle Frontiers in astronomy and space sciences
PublicationYear 2022
Publisher Frontiers Media S.A
Publisher_xml – name: Frontiers Media S.A
References Rozitis (B17) 2014; 512
Sánchez (B18) 2020; 338
Walsh (B27) 2018; 56
Maindl (B11) 2019; 6
Röstel (B16) 2020; 125
Keyak (B9) 2009; 44
de MoraisTeles (B6) 2015
Gasperi (B7) 20142014; 2014
O'Neill (B13) 1974; 27
Burns (B3) 1975; 25
Walsh (B26) 2019; 12
Pravec (B15) 2000; 148
Abe (B1) 2006; 312
O'Brien (B12) 2005; 178
Harris (B8) 2014; 9
Slyuta (B20) 1997; 129
Townsend (B23) 2020; 73
Sugita (B21) 2019; 364
Scheeres (B19) 2010; 210
Blamont (B2) 2014; 54
Lauretta (B10) 2019; 568
Chodas (B4) 2020
Paikowsky (B14) 2017; 5
Daly (B5) 2020; 6
Versari (B25) 2013; 27
Vedda (B24) 2019
Taibbi (B22) 2013; 84
References_xml – volume: 178
  start-page: 179
  year: 2005
  ident: B12
  article-title: The Collisional and Dynamical Evolution of the Main-belt and NEA Size Distributions
  publication-title: Icarus
  doi: 10.1016/j.icarus.2005.04.001
– volume: 512
  start-page: 174
  year: 2014
  ident: B17
  article-title: Cohesive Forces Prevent the Rotational Breakup of Rubble-Pile Asteroid (29075) 1950 DA
  publication-title: Nature
  doi: 10.1038/nature13632
– volume: 129
  start-page: 401
  year: 1997
  ident: B20
  article-title: Gravitational Deformation in Shaping Asteroids and Small Satellites
  publication-title: Icarus
  doi: 10.1006/icar.1997.5776
– volume: 25
  start-page: 545
  year: 1975
  ident: B3
  article-title: The Angular Momenta of Solar System Bodies: Implications for Asteroid Strengths
  publication-title: Icarus
  doi: 10.1016/0019-1035(75)90035-4
– volume: 5
  start-page: 84
  year: 2017
  ident: B14
  article-title: What Is New Space? the Changing Ecosystem of Global Space Activity
  publication-title: New Space
  doi: 10.1089/space.2016.0027
– volume: 364
  start-page: 252
  year: 2019
  ident: B21
  article-title: The Geomorphology, Color, and thermal Properties of Ryugu: Implications for Parent-Body Processes
  publication-title: Science
  doi: 10.1126/science.aaw0422
– volume: 125
  start-page: e06246
  year: 2020
  ident: B16
  article-title: Subsurface Radiation Environment of Mars and its Implication for Shielding Protection of Future Habitats
  publication-title: J. Geophys. Res. (Planets)
  doi: 10.1029/2019je006246
– volume: 9
  start-page: e106207
  year: 2014
  ident: B8
  article-title: How Much Gravity Is Needed to Establish the Perceptual Upright?
  publication-title: PLOS ONE
  doi: 10.1371/journal.pone.0106207
– volume: 6
  start-page: 37
  year: 2019
  ident: B11
  article-title: Stability of a Rotating Asteroid Housing a Space Station
  publication-title: Front. Astron. Space Sci.
  doi: 10.3389/fspas.2019.00037
– volume: 148
  start-page: 12
  year: 2000
  ident: B15
  article-title: Fast and Slow Rotation of Asteroids
  publication-title: Icarus
  doi: 10.1006/icar.2000.6482
– volume: 56
  start-page: 593
  year: 2018
  ident: B27
  article-title: Rubble Pile Asteroids
  publication-title: Annu. Rev. Astron. Astrophys.
  doi: 10.1146/annurev-astro-081817-052013
– start-page: 147
  volume-title: Planetary Exploration and Science: Recent Results and Advances
  year: 2015
  ident: B6
  article-title: Mars Astrobiology: Recent Status and Progress
  doi: 10.1007/978-3-662-45052-9_8
– volume: 44
  start-page: 449
  year: 2009
  ident: B9
  article-title: Reduction in Proximal Femoral Strength Due to Long-Duration Spaceflight
  publication-title: Bone
  doi: 10.1016/j.bone.2008.11.014
– volume: 27
  start-page: 32
  year: 1974
  ident: B13
  article-title: The Colonization of Space
  publication-title: Phys. Today
  doi: 10.1063/1.3128863
– year: 2020
  ident: B4
  article-title: Center for Near Earth Object Studies - Discovery Statistics
– volume: 84
  start-page: 148
  year: 2013
  ident: B22
  article-title: Effects of 30-day Head-Down Bed Rest on Ocular Structures and Visual Function in a Healthy Subject
  publication-title: Aviat Space Environ. Med.
  doi: 10.3357/asem.3520.2013
– volume: 2014
  start-page: 782390
  year: 20142014
  ident: B7
  article-title: A Functional Interplay between 5-lipoxygenase and μ-calpain Affects Survival and Cytokine Profile of Human Jurkat T Lymphocyte Exposed to Simulated Microgravity
  publication-title: Biomed. Res. Int.
  doi: 10.1155/2014/782390
– volume: 210
  start-page: 968
  year: 2010
  ident: B19
  article-title: Scaling Forces to Asteroid Surfaces: The Role of Cohesion
  publication-title: Icarus
  doi: 10.1016/j.icarus.2010.07.009
– volume: 568
  start-page: 55
  year: 2019
  ident: B10
  article-title: The Unexpected Surface of Asteroid (101955) Bennu
  publication-title: Nature
  doi: 10.1038/s41586-019-1033-6
– volume: 6
  start-page: eabd3649
  year: 2020
  ident: B5
  article-title: Hemispherical Differences in the Shape and Topography of Asteroid (101955) Bennu
  publication-title: Sci. Adv.
  doi: 10.1126/sciadv.abd3649
– volume: 54
  start-page: 2140
  year: 2014
  ident: B2
  article-title: A Roadmap to Cave Dwelling on the Moon and Mars
  publication-title: Adv. Space Res.
  doi: 10.1016/j.asr.2014.08.019
– volume: 312
  start-page: 1344
  year: 2006
  ident: B1
  article-title: Mass and Local Topography Measurements of Itokawa by Hayabusa
  publication-title: Science
  doi: 10.1126/science.1126272
– volume: 27
  start-page: 4466
  year: 2013
  ident: B25
  article-title: The Challenging Environment on Board the International Space Station Affects Endothelial Cell Function by Triggering Oxidative Stress through Thioredoxin Interacting Protein Overexpression: the ESA‐SPHINX experiment
  publication-title: FASEB j.
  doi: 10.1096/fj.13-229195
– volume-title: Space Leadership in Transition
  year: 2019
  ident: B24
– volume: 338
  start-page: 113443
  year: 2020
  ident: B18
  article-title: Cohesive Regolith on Fast Rotating Asteroids
  publication-title: Icarus
  doi: 10.1016/j.icarus.2019.113443
– volume: 73
  start-page: 66
  year: 2020
  ident: B23
  article-title: Space Weather on the Moon
  publication-title: Phys. Today
  doi: 10.1063/pt.3.4438
– volume: 12
  start-page: 242
  year: 2019
  ident: B26
  article-title: Craters, Boulders and Regolith of (101955) Bennu Indicative of an Old and Dynamic Surface
  publication-title: Nat. Geosci.
  doi: 10.1038/s41561-019-0326-6
SSID ssj0001878963
Score 2.169294
Snippet The authors explore the possibility that near-earth, rubble pile asteroids might be used as habitats for human settlement by increasing their rotation to...
SourceID doaj
crossref
SourceType Open Website
Index Database
SubjectTerms finite element analysis
habitat design
hoop stress
near earth asteroids
numerical simulations
rubble pile asteroids
Title Habitat Bennu: Design Concepts for Spinning Habitats Constructed From Rubble Pile Near-Earth Asteroids
URI https://doaj.org/article/bd0ed441cdb6473bb5aec0f4b38b68e8
Volume 8
hasFullText 1
inHoldings 1
isFullTextHit
isPrint
link http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwrV1LSwMxEA7SkxfxSeuLHMSDsDbdZJOtt7ZaimARtdDbktkkWLAPuu3Bf-8kqVJPXrwt2ZBdvpnJTB7zDSFXUCpeGhCJ0zz1JcxkAjnoRMnSZsyK1IXjgqehHIzE4zgbb5X68nfCIj1wBK4JhlmDPhsHlEJxgEzbkjkBPAeZ25Dmiz5vazEVdldylaNqxWNMXIW1mw4N1NNzp61bKTIu-S9HtMXXHxxLf5_sbSJC2ol_ckB27OyQ1DuV36OeTz_pNQ3PcQuiOiJuoMEnhtEuzpHrO3of7mDQXsw_rChGofR1MQmliOimb-VfR6pYa2h_OZ_SlzXAh6XPOCvQIap78oBYvPtv2eV8YqpjMuo_vPUGyaZaQlJi2L9KWqVuezp5hNdpnQnp0PcblJEySqfCtLw9M2dzbmQGaNeageGSWYxBlGGGn5DabD6zdUJLwTSTWnOfFauyDDBGlO2UaaPASKca5OYbumIRSTEKXEx4nIuAc-FxLiLODdL14P509HzWoQGlXGykXPwl5dP_GOSM7KY-eSFcIjsnNUTdXmBIsYLLoD1fkJbMeg
linkProvider Directory of Open Access Journals
openUrl ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Habitat+Bennu%3A+Design+Concepts+for+Spinning+Habitats+Constructed+From+Rubble+Pile+Near-Earth+Asteroids&rft.jtitle=Frontiers+in+astronomy+and+space+sciences&rft.au=Miklav%C4%8Di%C4%8D%2C+Peter+M.&rft.au=Siu%2C+John&rft.au=Wright%2C+Esteban&rft.au=Debrecht%2C+Alex&rft.date=2022-01-03&rft.issn=2296-987X&rft.eissn=2296-987X&rft.volume=8&rft_id=info:doi/10.3389%2Ffspas.2021.645363&rft.externalDBID=n%2Fa&rft.externalDocID=10_3389_fspas_2021_645363
thumbnail_l http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=2296-987X&client=summon
thumbnail_m http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=2296-987X&client=summon
thumbnail_s http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=2296-987X&client=summon