migration in the Solar system

Renu Malhotra Lunar and Planetary Laboratory The University of Arizona

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Planet migration in the Solar system

Renu Malhotra Lunar and Planetary Laboratory The University of Arizona

•The solar system has not always looked like it does now (@ age of 4.567 Gy) @ 4.5 Gyr ago: orbits more compact + a lot more debris (, ) @ 3.9 Gyr ago: debris cleared up (mostly), seled into their present orbits

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 A little bit about me …

I am interested in the “architecture” of planetary systems - how planetary masses and orbits are arranged - how they form and change over time

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 A little bit about me …

I am interested in the “architecture” of planetary systems - how planetary masses and orbits are arranged - how they form and change over time

physics + + mathematics

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 my own peregrinations…

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 New Delhi my own peregrinations… +various 1961-1968

Hyderabad 1968-1978

New Delhi 1978-1983

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 St. Ann’s School, Secunderabad, India

all-girls school

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 St. Ann’s School, Secunderabad, India

all-girls school

Indian Institute of Technology, Delhi ~3% !

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 St. Ann’s School, Secunderabad, India

all-girls school

Indian Institute of Technology, Delhi ~3% !

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Ithaca, NY Cornell Univ 1983-1989

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Urbana, IL 1991-1993 Ithaca, NY 1983-1989

Pasadena, CA 1989-1991 India

Houston, TX 1991-2000 Tucson, AZ 2000-

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Urbana, IL 1991-1993 Ithaca, NY 1983-1989

Pasadena, CA 1989-1991 India

Houston, TX 1991-2000 Tucson, AZ 2000-

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Undergraduate: Physics

Graduate studies: Physics

Dynamical systems - chaos theory

Planetary dynamics/planetary science

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 factors that have been important in my life and career

- adversity & serendipity

- curiosity - broad-minded parents - ignoring distractions - teachers & mentors - perseverance - partner - perfectionism - USA ... country & society

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 On to planets…

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Ancient concept of cosmos eternal, Celestial sphere unchanging in time

planets

Sun

Moon

Earth

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Modern concept of the cosmos

Earth is a planet in the solar system … in the Milky Way Galaxy … in the Local Cluster of galaxies … in the Universe

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Modern concept of the cosmos

Earth is a planet in the solar system … in the Milky Way Galaxy … in the Local Cluster of galaxies … in the Universe

evolves on many timescales

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Four or Five distinct neighborhoods in the Solar system also some stragglers in-between (NEOs, Centaurs)

Oort Cloud

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Four or Five distinct neighborhoods in the Solar system also some stragglers in-between (NEOs, Centaurs)

Oort Cloud

You are here

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 circa ~1990 … Nine planets in the solar system

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Pluto is eccentric its orbital path overlaps that of Neptune but it is in no danger of colliding with Neptune

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Pluto is eccentric its orbital path overlaps that of Neptune but it is in no danger of colliding with Neptune

Rotating frame

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Pluto is eccentric its orbital path overlaps that of Neptune but it is in no danger of colliding with Neptune

Rotating frame

20,000 year libration

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Neptune’s migration and Resonance sweeping

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Neptune’s migration and Resonance sweeping

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Neptune’s migration and Resonance sweeping

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Neptune’s migration and Resonance sweeping

Prediction: pile-ups of KBOs in resonances

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Giant planet migration fueled by leftover planetesimals

ejected Oort scattered Cloud

solar system @ ~4 Ga

solar system ~today

cleared surviving debris

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Planetesimal clearing ➡ back-reaction on the planets

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Planetesimal clearing ➡ back-reaction on the planets

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Planetesimal clearing ➡ back-reaction on the planets

Jupiter…Neptune + trillions of planetesimals ➡ migrates inward, Neptune migrates outward

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Pluto’s resonance Neptune’s and eccentricity migration

eP = 0.25 ⇒ ΔaN ≳ 5 au Confirmed with computer simulations

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18

© 1993 Nature Publishing Group

© 1993 Nature Publishing Group Kuiper Belt observations eccentricity

semi-major axis, au

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Kuiper Belt observations

resonances, eccentricities, inclinations ➡ Neptune migrated out ≳10AU eccentricity

semi-major axis, au

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Other observational tests?

Asteroid belt Impact craters on planetary surfaces

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 belt - Kirkwood gaps

image: wikipedia

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 - Kirkwood gaps

Discovered by Daniel Kirkwood

in 1857, when less than 100 asteroids were known image: wikipedia Kirkwood related the locations of the gaps to mean motion resonances w/Jupiter

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Asteroid belt - Kirkwood gaps

Discovered by Daniel Kirkwood

in 1857, when less than 100 asteroids were known image: wikipedia Kirkwood related the locations of the gaps to mean motion resonances w/Jupiter

The gaps sizes are best explained if Jupiter migrated inward from a slightly larger orbit renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Clues in the impact crater record - two different populations of craters Moon

Mercury

Mars

Venus

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Clues in the impact crater record - two different populations of craters Moon

Mercury

Mars

Venus

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18 Summary

• The solar system has not always looked like it does now (@ age of 4.567 Gy) @ 4.5 Gyr ago: orbits more compact + a lot more debris (asteroids, comets) @ ~4 Gyr ago: debris cleared up (mostly), planets settled into their present orbits

• That early dynamic period had major consequences ✦ planetary re-arrangements ⇒ (more) stable orbits ✦ heavy meteoroidal bombardment ✦ very little asteroidal/cometary debris left, hence low bombardment rate on Earth

•Details under active study and debate

renu malhotra/LPL, U of Arizona CUWiP-Univ of Oklahoma-2020-jan-18