DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The structure of terrestrial bodies: Impact heating, corotation limits, and synestias

Abstract

During accretion, terrestrial bodies attain a wide range of thermal and rotational states, which are accompanied by significant changes in physical structure (size, shape, pressure and temperature profile, etc.). However, variations in structure have been neglected in most studies of rocky planet formation and evolution. Here we present a new code, the Highly Eccentric Rotating Concentric U (potential) Layers Equilibrium Structure (HERCULES) code, that solves for the equilibrium structure of planets as a series of overlapping constant-density spheroids. Using HERCULES and a smoothed particle hydrodynamics code, we show that Earth-like bodies display a dramatic range of morphologies. For any rotating planetary body, there is a thermal limit beyond which the rotational velocity at the equator intersects the Keplerian orbital velocity. Beyond this corotation limit (CoRoL), a hot planetary body forms a structure, which we name a synestia, with a corotating inner region connected to a disk-like outer region. By analyzing calculations of giant impacts and models of planet formation, we show that typical rocky planets are substantially vaporized multiple times during accretion. For the expected angular momentum of growing planets, a large fraction of post-impact bodies will exceed the CoRoL and form synestias. The common occurrence of hot, rotating statesmore » during accretion has major implications for planet formation and the properties of the final planets. In particular, the structure of post-impact bodies influences the physical processes that control accretion, core formation, and internal evolution. Synestias also lead to new mechanisms for satellite formation. Finally, the wide variety of possible structures for terrestrial bodies also expands the mass-radius range for rocky exoplanets.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]
  1. Harvard Univ., Cambridge, MA (United States)
  2. Univ. of California, Davis, CA (United States)
Publication Date:
Research Org.:
Harvard Univ., Cambridge, MA (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA)
OSTI Identifier:
1532991
Alternate Identifier(s):
OSTI ID: 1788246
Grant/Contract Number:  
NA0001804; NA0002937
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Geophysical Research. Planets
Additional Journal Information:
Journal Volume: 122; Journal Issue: 5; Journal ID: ISSN 2169-9097
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
58 GEOSCIENCES; Geochemistry & Geophysics

Citation Formats

Lock, Simon J., and Stewart, Sarah T. The structure of terrestrial bodies: Impact heating, corotation limits, and synestias. United States: N. p., 2017. Web. doi:10.1002/2016je005239.
Lock, Simon J., & Stewart, Sarah T. The structure of terrestrial bodies: Impact heating, corotation limits, and synestias. United States. https://doi.org/10.1002/2016je005239
Lock, Simon J., and Stewart, Sarah T. Mon . "The structure of terrestrial bodies: Impact heating, corotation limits, and synestias". United States. https://doi.org/10.1002/2016je005239. https://www.osti.gov/servlets/purl/1532991.
@article{osti_1532991,
title = {The structure of terrestrial bodies: Impact heating, corotation limits, and synestias},
author = {Lock, Simon J. and Stewart, Sarah T.},
abstractNote = {During accretion, terrestrial bodies attain a wide range of thermal and rotational states, which are accompanied by significant changes in physical structure (size, shape, pressure and temperature profile, etc.). However, variations in structure have been neglected in most studies of rocky planet formation and evolution. Here we present a new code, the Highly Eccentric Rotating Concentric U (potential) Layers Equilibrium Structure (HERCULES) code, that solves for the equilibrium structure of planets as a series of overlapping constant-density spheroids. Using HERCULES and a smoothed particle hydrodynamics code, we show that Earth-like bodies display a dramatic range of morphologies. For any rotating planetary body, there is a thermal limit beyond which the rotational velocity at the equator intersects the Keplerian orbital velocity. Beyond this corotation limit (CoRoL), a hot planetary body forms a structure, which we name a synestia, with a corotating inner region connected to a disk-like outer region. By analyzing calculations of giant impacts and models of planet formation, we show that typical rocky planets are substantially vaporized multiple times during accretion. For the expected angular momentum of growing planets, a large fraction of post-impact bodies will exceed the CoRoL and form synestias. The common occurrence of hot, rotating states during accretion has major implications for planet formation and the properties of the final planets. In particular, the structure of post-impact bodies influences the physical processes that control accretion, core formation, and internal evolution. Synestias also lead to new mechanisms for satellite formation. Finally, the wide variety of possible structures for terrestrial bodies also expands the mass-radius range for rocky exoplanets.},
doi = {10.1002/2016je005239},
journal = {Journal of Geophysical Research. Planets},
number = 5,
volume = 122,
place = {United States},
year = {Mon May 22 00:00:00 EDT 2017},
month = {Mon May 22 00:00:00 EDT 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 66 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

Accretion of the Earth
journal, September 2008

  • Canup, Robin M.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 366, Issue 1883
  • DOI: 10.1098/rsta.2008.0101

Collisions Between Gravity-Dominated Bodies. i. Outcome Regimes and Scaling laws
journal, December 2011


A Numerical Study of the Stability of Flattened Galaxies: or, can Cold Galaxies Survive?
journal, December 1973

  • Ostriker, J. P.; Peebles, P. J. E.
  • The Astrophysical Journal, Vol. 186
  • DOI: 10.1086/152513

Concentric Maclaurin Spheroid Models of Rotating Liquid Planets
journal, April 2013


Gravitational instability in two-phase disks and the origin of the moon
journal, October 1988

  • Thompson, Christopher; Stevenson, David J.
  • The Astrophysical Journal, Vol. 333
  • DOI: 10.1086/166760

Evidence for multiple magma ocean outgassing and atmospheric loss episodes from mantle noble gases
journal, May 2014


Rapidly Rotating Stars. II. Massive White Dwarfs
journal, January 1968

  • Ostriker, Jeremiah P.; Bodenheimer, Peter
  • The Astrophysical Journal, Vol. 151
  • DOI: 10.1086/149507

Circumplanetary disk Formation
journal, October 2010


High-temperature miscibility of iron and rock during terrestrial planet formation
journal, January 2015


Growing the terrestrial planets from the gradual accumulation of submeter-sized objects
journal, October 2015

  • Levison, Harold F.; Kretke, Katherine A.; Walsh, Kevin J.
  • Proceedings of the National Academy of Sciences, Vol. 112, Issue 46
  • DOI: 10.1073/pnas.1513364112

Rocky Planet Formation: Quick and neat
journal, October 2016

  • Kenyon, Scott J.; Najita, Joan R.; Bromley, Benjamin C.
  • The Astrophysical Journal, Vol. 831, Issue 1
  • DOI: 10.3847/0004-637X/831/1/8

An early geodynamo driven by exsolution of mantle components from Earth’s core
journal, July 2016

  • Badro, James; Siebert, Julien; Nimmo, Francis
  • Nature, Vol. 536, Issue 7616
  • DOI: 10.1038/nature18594

Rapidly Rotating Stars. VII. Effects of Angular Momentum on Upper-Main Models
journal, July 1971

  • Bodenheimer, Peter
  • The Astrophysical Journal, Vol. 167
  • DOI: 10.1086/151014

The Structure and Stability of Rotating Gas Masses.
journal, August 1964

  • James, R. A.
  • The Astrophysical Journal, Vol. 140
  • DOI: 10.1086/147949

Thermal evolution of Earth with magnesium precipitation in the core
journal, January 2017

  • O'Rourke, Joseph G.; Korenaga, Jun; Stevenson, David J.
  • Earth and Planetary Science Letters, Vol. 458
  • DOI: 10.1016/j.epsl.2016.10.057

Compositional Evolution During Rocky Protoplanet Accretion
journal, October 2015

  • Carter, Philip. J.; Leinhardt, Zoë. M.; Elliott, Tim
  • The Astrophysical Journal, Vol. 813, Issue 1
  • DOI: 10.1088/0004-637X/813/1/72

On the convergence of the theory of figures
journal, November 2014


Internal structure of massive terrestrial planets
journal, April 2006


Atmospheric mass loss during planet formation: The importance of planetesimal impacts
journal, February 2015


High-Precision Maclaurin-Based Models of Rotating Liquid Planets
journal, August 2012


Formation and Destruction of Small Binary Asteroids
journal, March 2007

  • Ćuk, Matija
  • The Astrophysical Journal, Vol. 659, Issue 1
  • DOI: 10.1086/516572

Dating the Moon-forming impact event with asteroidal meteorites
journal, April 2015


Decaying shock studies of phase transitions in MgO-SiO 2 systems: Implications for the super-Earths' interiors : Decaying Shock in MgO-SiO
journal, September 2016

  • Bolis, R. M.; Morard, G.; Vinci, T.
  • Geophysical Research Letters, Vol. 43, Issue 18
  • DOI: 10.1002/2016GL070466

A Detailed Model Grid for Solid Planets from 0.1 through 100 Earth Masses
journal, March 2013

  • Zeng, Li; Sasselov, Dimitar
  • Publications of the Astronomical Society of the Pacific, Vol. 125, Issue 925
  • DOI: 10.1086/669163

Mass–Radius Relation for Rocky Planets Based on prem
journal, March 2016


Mass-Radius Relationships for Exoplanets
journal, December 2011


Shock compression response of forsterite above 250 GPa
journal, August 2016

  • Sekine, Toshimori; Ozaki, Norimasa; Miyanishi, Kohei
  • Science Advances, Vol. 2, Issue 8
  • DOI: 10.1126/sciadv.1600157

On the evolution of the protolunar disc
journal, September 2014

  • Ward, William R.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 372, Issue 2024
  • DOI: 10.1098/rsta.2013.0250

The Mass-Radius Relation for 65 Exoplanets Smaller than 4 Earth Radii
journal, February 2014


CHARACTERISTICS OF PLANETARY CANDIDATES OBSERVED BY KEPLER . II. ANALYSIS OF THE FIRST FOUR MONTHS OF DATA
journal, June 2011


Accretion of the Moon from non-canonical discs
journal, September 2014

  • Salmon, J.; Canup, R. M.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 372, Issue 2024
  • DOI: 10.1098/rsta.2013.0256

Equilibrium figures of spinning bodies with self-gravity
journal, November 2004


A low mass for Mars from Jupiter’s early gas-driven migration
journal, June 2011

  • Walsh, Kevin J.; Morbidelli, Alessandro; Raymond, Sean N.
  • Nature, Vol. 475, Issue 7355
  • DOI: 10.1038/nature10201

A Scaling Relationship for Satellite-Forming Impacts
journal, April 2001


Lunar-forming impacts: High-resolution SPH and AMR-CTH simulations
journal, January 2013


Angular Momentum Evolution of Young Stars and Disks
journal, September 1995


Early differentiation and volatile accretion recorded in deep-mantle neon and xenon
journal, June 2012


Melting of Iron at Earth's Inner Core Boundary Based on Fast X-ray Diffraction
journal, April 2013


Origin of the Moon in a giant impact near the end of the Earth's formation
journal, August 2001

  • Canup, Robin M.; Asphaug, Erik
  • Nature, Vol. 412, Issue 6848
  • DOI: 10.1038/35089010

Evolution of a protolunar disk in vapor/melt equilibrium: Vapor-Melt Disk
journal, February 2017

  • Ward, William R.
  • Journal of Geophysical Research: Planets, Vol. 122, Issue 2
  • DOI: 10.1002/2016JE005198

Lunar volatile depletion due to incomplete accretion within an impact-generated disk
journal, November 2015

  • Canup, Robin M.; Visscher, Channon; Salmon, Julien
  • Nature Geoscience, Vol. 8, Issue 12
  • DOI: 10.1038/ngeo2574

Lunar accretion from an impact-generated disk
journal, September 1997

  • Ida, Shigeru; Canup, Robin M.; Stewart, Glen R.
  • Nature, Vol. 389, Issue 6649
  • DOI: 10.1038/38669

Collisions Between Gravity-Dominated Bodies. ii. the Diversity of Impact Outcomes During the end Stage of Planet Formation
journal, May 2012


Enhanced atmospheric loss on protoplanets at the giant impact phase in the presence of oceans
journal, February 2005


MOST 1.6 EARTH-RADIUS PLANETS ARE NOT ROCKY
journal, March 2015


Melting and mixing states of the Earth's mantle after the Moon-forming impact
journal, October 2015


A hydrocode equation of state for SiO 2
journal, December 2007


Binary asteroid population
journal, September 2007


Collisional Stripping and Disruption of Super-Earths
journal, July 2009


Formation of Terrestrial Planets from Protoplanets. II. Statistics of Planetary Spin
journal, December 2007

  • Kokubo, Eiichiro; Ida, Shigeru
  • The Astrophysical Journal, Vol. 671, Issue 2
  • DOI: 10.1086/522364

Magma ocean influence on early atmosphere mass and composition
journal, August 2012


Numerical experiments with rubble piles: equilibrium shapes and spins
journal, February 2005


The heavy noble gas composition of the depleted MORB mantle (DMM) and its implications for the preservation of heterogeneities in the mantle
journal, November 2012

  • Tucker, Jonathan M.; Mukhopadhyay, Sujoy; Schilling, Jean-Guy
  • Earth and Planetary Science Letters, Vol. 355-356
  • DOI: 10.1016/j.epsl.2012.08.025

Scaling the Earth: a Sensitivity Analysis of Terrestrial Exoplanetary Interior Models
journal, February 2016


Equilibration in the aftermath of the lunar-forming giant impact
journal, October 2007


The cosmological simulation code gadget-2
journal, December 2005


Formation and Evolution of Binary Asteroids
book, January 2015


Terrestrial Planet Formation
conference, January 2004

  • Chambers, John E.
  • THE SEARCH FOR OTHER WORLDS: Fourteenth Astrophysics Conference, AIP Conference Proceedings
  • DOI: 10.1063/1.1774526

Heterogeneities from the first 100 million years recorded in deep mantle noble gases from the Northern Lau Back-arc Basin
journal, May 2013

  • Pető, Maria K.; Mukhopadhyay, Sujoy; Kelley, Katherine A.
  • Earth and Planetary Science Letters, Vol. 369-370
  • DOI: 10.1016/j.epsl.2013.02.012

Heterogeneous upper mantle Ne, Ar and Xe isotopic compositions and a possible Dupal noble gas signature recorded in basalts from the Southwest Indian Ridge
journal, December 2012


Powering Earth’s dynamo with magnesium precipitation from the core
journal, January 2016

  • O’Rourke, Joseph G.; Stevenson, David J.
  • Nature, Vol. 529, Issue 7586
  • DOI: 10.1038/nature16495

Shock vaporization of silica and the thermodynamics of planetary impact events: SHOCK VAPORIZATION OF SILICA
journal, September 2012

  • Kraus, R. G.; Stewart, S. T.; Swift, D. C.
  • Journal of Geophysical Research: Planets, Vol. 117, Issue E9
  • DOI: 10.1029/2012JE004082

Early Earth differentiation investigated through 142Nd, 182W, and highly siderophile element abundances in samples from Isua, Greenland
journal, February 2016


On the Vertical Structure of the Protolunar disk
journal, December 2011


Thermal evolution of an early magma ocean in interaction with the atmosphere: MAGMA OCEAN AND ATMOSPHERE EVOLUTION
journal, June 2013

  • Lebrun, T.; Massol, H.; Chassefière, E.
  • Journal of Geophysical Research: Planets, Vol. 118, Issue 6
  • DOI: 10.1002/jgre.20068

FALSE POSITIVE PROBABILITIES FOR ALL KEPLER OBJECTS OF INTEREST: 1284 NEWLY VALIDATED PLANETS AND 428 LIKELY FALSE POSITIVES
journal, May 2016

  • Morton, Timothy D.; Bryson, Stephen T.; Coughlin, Jeffrey L.
  • The Astrophysical Journal, Vol. 822, Issue 2
  • DOI: 10.3847/0004-637X/822/2/86

Early evolution of the Earth–Moon system with a fast-spinning Earth
journal, August 2015


Evolution of the Earth-Moon system
journal, November 1994

  • Touma, Jihad; Wisdom, Jack
  • The Astronomical Journal, Vol. 108
  • DOI: 10.1086/117209

Evolution of a Circumterrestrial Disk and Formation of a Single Moon
journal, December 2000


Building the terrestrial planets: Constrained accretion in the inner Solar System
journal, October 2009


Emergence of a Habitable Planet
journal, July 2007


Lunar Accretion from a Roche-Interior Fluid disk
journal, November 2012


Lunar-forming collisions with pre-impact rotation
journal, August 2008


Tidal evolution of the Moon from a high-obliquity, high-angular-momentum Earth
journal, October 2016

  • Ćuk, Matija; Hamilton, Douglas P.; Lock, Simon J.
  • Nature, Vol. 539, Issue 7629
  • DOI: 10.1038/nature19846

Simulations of a late lunar-forming impact
journal, April 2004


Terrestrial planet formation with strong dynamical friction
journal, September 2006


On the Oscillations and Stability of Rotating Stellar Models. II. Rapidly Rotating White Dwarfs
journal, February 1969

  • Ostriker, Jeremiah P.; Tassoul, Jean Louis
  • The Astrophysical Journal, Vol. 155
  • DOI: 10.1086/149927

Rotational breakup as the origin of small binary asteroids
journal, July 2008

  • Walsh, Kevin J.; Richardson, Derek C.; Michel, Patrick
  • Nature, Vol. 454, Issue 7201
  • DOI: 10.1038/nature07078

Binary Minor Planets
journal, May 2006


Isotopic Composition of the Moon and the Lunar Isotopic Crisis
book, January 2014


Satellite-sized planetesimals and lunar origin
journal, April 1975


TRANSITS AND OCCULTATIONS OF AN EARTH-SIZED PLANET IN AN 8.5 hr ORBIT
journal, August 2013

  • Sanchis-Ojeda, Roberto; Rappaport, Saul; Winn, Joshua N.
  • The Astrophysical Journal, Vol. 774, Issue 1
  • DOI: 10.1088/0004-637X/774/1/54

On the Gravitational Fields of Maclaurin Spheroid Models of Rotating Fluid Planets
journal, January 2013


Mass‐Radius Relationships for Solid Exoplanets
journal, November 2007

  • Seager, S.; Kuchner, M.; Hier‐Majumder, C. A.
  • The Astrophysical Journal, Vol. 669, Issue 2
  • DOI: 10.1086/521346

Potassium isotopic evidence for a high-energy giant impact origin of the Moon
journal, September 2016


Debris from terrestrial planet formation: the Moon-forming collision: Debris from terrestrial planet formation
journal, August 2012


On the Oscillations and Stability of Rapidly Rotating Stellar Models. 111. Zero-Viscosity Polytropic Sequences
journal, February 1973

  • Ostriker, Jeremiah P.; Bodenheimer, Peter
  • The Astrophysical Journal, Vol. 180
  • DOI: 10.1086/151952

A map of the large day–night temperature gradient of a super-Earth exoplanet
journal, March 2016

  • Demory, Brice-Olivier; Gillon, Michael; de Wit, Julien
  • Nature, Vol. 532, Issue 7598
  • DOI: 10.1038/nature17169

The Origin of the Natural Satellites
book, January 2015


The Frequency of Giant Impacts on Earth-Like Worlds
journal, April 2016

  • Quintana, Elisa V.; Barclay, Thomas; Borucki, William J.
  • The Astrophysical Journal, Vol. 821, Issue 2
  • DOI: 10.3847/0004-637X/821/2/126

Forming a Moon with an Earth-like Composition via a Giant Impact
journal, October 2012


The Evolution of an Impact‐generated Partially Vaporized Circumplanetary Disk
journal, December 2004

  • Machida, Ryosuke; Abe, Yutaka
  • The Astrophysical Journal, Vol. 617, Issue 1
  • DOI: 10.1086/425209

Coupled orbital-thermal evolution of the early Earth-Moon system with a fast-spinning Earth
journal, January 2017


Making the Moon from a Fast-Spinning Earth: A Giant Impact Followed by Resonant Despinning
journal, October 2012


Formation of the Terrestrial Planets from a Narrow Annulus
journal, September 2009


New approaches to the Moon's isotopic crisis
journal, September 2014

  • Melosh, H. J.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 372, Issue 2024
  • DOI: 10.1098/rsta.2013.0168

Works referencing / citing this record:

Time‐Dependent Hybrid Plasma Simulations of Lunar Electromagnetic Induction in the Solar Wind
journal, April 2019

  • Fuqua Haviland, H.; Poppe, A. R.; Fatemi, S.
  • Geophysical Research Letters, Vol. 46, Issue 8
  • DOI: 10.1029/2018gl080523

Modeling a Transient Secondary Paleolunar Atmosphere: 3‐D Simulations and Analysis
journal, May 2019

  • Aleinov, I.; Way, M. J.; Harman, C.
  • Geophysical Research Letters, Vol. 46, Issue 10
  • DOI: 10.1029/2019gl082494

Shock compression of fused silica: An impedance matching standard
journal, October 2019

  • Root, Seth; Townsend, Joshua P.; Knudson, Marcus D.
  • Journal of Applied Physics, Vol. 126, Issue 16
  • DOI: 10.1063/1.5126205

Rayleigh–Taylor instabilities in high-energy density settings on the National Ignition Facility
journal, June 2018

  • Remington, Bruce A.; Park, Hye-Sook; Casey, Daniel T.
  • Proceedings of the National Academy of Sciences, Vol. 116, Issue 37
  • DOI: 10.1073/pnas.1717236115

Oxygen isotopic evidence for accretion of Earth’s water before a high-energy Moon-forming giant impact
journal, March 2018

  • Greenwood, Richard C.; Barrat, Jean-Alix; Miller, Martin F.
  • Science Advances, Vol. 4, Issue 3
  • DOI: 10.1126/sciadv.aao5928

Giant impacts stochastically change the internal pressures of terrestrial planets
journal, September 2019


Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
journal, April 2019

  • Su, Kate Y. L.; Jackson, Alan P.; Gáspár, András
  • The Astronomical Journal, Vol. 157, Issue 5
  • DOI: 10.3847/1538-3881/ab1260

The Role of Multiple Giant Impacts in the Formation of the Earth–Moon System
journal, July 2018

  • Citron, Robert I.; Perets, Hagai B.; Aharonson, Oded
  • The Astrophysical Journal, Vol. 862, Issue 1
  • DOI: 10.3847/1538-4357/aaca2d

Primordial Earth Mantle Heterogeneity Caused by the Moon-forming Giant Impact?
journal, December 2019

  • Deng, Hongping; Ballmer, Maxim D.; Reinhardt, Christian
  • The Astrophysical Journal, Vol. 887, Issue 2
  • DOI: 10.3847/1538-4357/ab50b9

Primordial Earth Mantle Heterogeneity Caused by the Moon-forming Giant Impact?
text, January 2019

  • Deng, Hongping; Ballmer, Maxim D.; Reinhardt, Christian
  • IOP Publishing
  • DOI: 10.5167/uzh-182528

The energy budgets of giant impacts
text, January 2019