Solar Wind Plasma Interaction with Asteroid 16 Psyche: Implication for Formation Theories. Issue 1 (8th January 2018)
- Record Type:
- Journal Article
- Title:
- Solar Wind Plasma Interaction with Asteroid 16 Psyche: Implication for Formation Theories. Issue 1 (8th January 2018)
- Main Title:
- Solar Wind Plasma Interaction with Asteroid 16 Psyche: Implication for Formation Theories
- Authors:
- Fatemi, Shahab
Poppe, Andrew R. - Abstract:
- Abstract: The asteroid 16 Psyche is a primitive metal‐rich asteroid that has not yet been visited by spacecraft. Based on remote observations, Psyche is most likely composed of iron and nickel metal; however, the history of its formation and solidification is still unknown. If Psyche is a remnant core of a differentiated planetesimal exposed by collisions, it opens a unique window toward understanding the cores of the terrestrial bodies, including the Earth and Mercury. If not, it is perhaps a reaccreted rubble pile that has never melted. In the former case, Psyche may have a remanent, dipolar magnetic field; in the latter case, Psyche may have no intrinsic field, but nevertheless would be a conductive object in the solar wind. We use Advanced Modeling Infrastructure in Space Simulation (AMITIS), a three‐dimensional GPU‐based hybrid model of plasma that self‐consistently couples the interior electromagnetic response of Psyche (i.e., magnetic diffusion) to its ambient plasma environment in order to quantify the different interactions under these two cases. The model results provide estimates for the electromagnetic environment of Psyche, showing that the magnetized case and the conductive case present very different signatures in the solar wind. These results have implications for an accurate interpretation of magnetic field observations by NASA's Discovery mission (Psyche mission) to the asteroid 16 Psyche. Key Points: Hybrid simulations of solar wind plasma interaction withAbstract: The asteroid 16 Psyche is a primitive metal‐rich asteroid that has not yet been visited by spacecraft. Based on remote observations, Psyche is most likely composed of iron and nickel metal; however, the history of its formation and solidification is still unknown. If Psyche is a remnant core of a differentiated planetesimal exposed by collisions, it opens a unique window toward understanding the cores of the terrestrial bodies, including the Earth and Mercury. If not, it is perhaps a reaccreted rubble pile that has never melted. In the former case, Psyche may have a remanent, dipolar magnetic field; in the latter case, Psyche may have no intrinsic field, but nevertheless would be a conductive object in the solar wind. We use Advanced Modeling Infrastructure in Space Simulation (AMITIS), a three‐dimensional GPU‐based hybrid model of plasma that self‐consistently couples the interior electromagnetic response of Psyche (i.e., magnetic diffusion) to its ambient plasma environment in order to quantify the different interactions under these two cases. The model results provide estimates for the electromagnetic environment of Psyche, showing that the magnetized case and the conductive case present very different signatures in the solar wind. These results have implications for an accurate interpretation of magnetic field observations by NASA's Discovery mission (Psyche mission) to the asteroid 16 Psyche. Key Points: Hybrid simulations of solar wind plasma interaction with magnetized or conductive asteroid Psyche Magnetized and conductive cases for Psyche show significant differences in solar wind interaction We provide predictions for Discovery mission to Psyche with implications for the formation history of Psyche … (more)
- Is Part Of:
- Geophysical research letters. Volume 45:Issue 1(2018)
- Journal:
- Geophysical research letters
- Issue:
- Volume 45:Issue 1(2018)
- Issue Display:
- Volume 45, Issue 1 (2018)
- Year:
- 2018
- Volume:
- 45
- Issue:
- 1
- Issue Sort Value:
- 2018-0045-0001-0000
- Page Start:
- 39
- Page End:
- 48
- Publication Date:
- 2018-01-08
- Subjects:
- 16 Psyche -- Solar wind interactions -- Hybrid simulations -- Interaction with conductive objects -- Interaction with magnetized objects
Geophysics -- Periodicals
Planets -- Periodicals
Lunar geology -- Periodicals
550 - Journal URLs:
- http://www.agu.org/journals/gl/ ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1002/2017GL073980 ↗
- Languages:
- English
- ISSNs:
- 0094-8276
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4156.900000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 8978.xml