arXiv Open Access 2025

A One-Dimensional Energy Balance Model Parameterization for the Formation of CO2 Ice on the Surfaces of Eccentric Extrasolar Planets

Vidya Venkatesan Aomawa L. Shields Russell Deitrick Eric T. Wolf Andrew Rushby +31 lainnya
Lihat Sumber

Abstrak

Eccentric planets may spend a significant portion of their orbits at large distances from their host stars, where low temperatures can cause atmospheric CO2 to condense out onto the surface, similar to the polar ice caps on Mars. The radiative effects on the climates of these planets throughout their orbits would depend on the wavelength-dependent albedo of surface CO2 ice that may accumulate at or near apoastron and vary according to the spectral energy distribution of the host star. To explore these possible effects, we incorporated a CO2 ice-albedo parameterization into a one-dimensional energy balance climate model. With the inclusion of this parameterization, our simulations demonstrated that F-dwarf planets require 29% more orbit-averaged flux to thaw out of global water ice cover compared with simulations that solely use a traditional pure water ice-albedo parameterization. When no eccentricity is assumed, and host stars are varied, F-dwarf planets with higher bond albedos relative to their M-dwarf planet counterparts require 30% more orbit-averaged flux to exit a water snowball state. Additionally, the intense heat experienced at periastron aids eccentric planets in exiting a snowball state with a smaller increase in instellation compared with planets on circular orbits; this enables eccentric planets to exhibit warmer conditions along a broad range of instellation. This study emphasizes the significance of incorporating an albedo parameterization for the formation of CO2 ice into climate models to accurately assess the habitability of eccentric planets, as we show that, even at moderate eccentricities, planets with Earth-like atmospheres can reach surface temperatures cold enough for the condensation of CO2 onto their surfaces, as can planets receiving low amounts of instellation on circular orbits.

Topik & Kata Kunci

Penulis (36)

V

Vidya Venkatesan

A

Aomawa L. Shields

R

Russell Deitrick

E

Eric T. Wolf

A

Andrew Rushby

D

Department of Physics

Astronomy

U

University of California

Irvine

California

USA

S

School of Earth

O

Ocean Sciences

U

University of Victoria

Victoria

Canada

L

Laboratory for Atmospheric

S

Space Physics

U

University of Colorado Boulder

Boulder

Colorado

USA

S

Sellers Exoplanet Environment Collaboration

N

NASA Goddard Space Flight Center

Greenbelt

Maryland

USA

B

Blue Marble Space Institute of Science

Seattle

Washington

USA

D

Department of Earth

P

Planetary Sciences

B

Birkbeck University of London

London

U

United Kingdom

Format Sitasi

Venkatesan, V., Shields, A.L., Deitrick, R., Wolf, E.T., Rushby, A., Physics, D.o. et al. (2025). A One-Dimensional Energy Balance Model Parameterization for the Formation of CO2 Ice on the Surfaces of Eccentric Extrasolar Planets. https://arxiv.org/abs/2501.11667

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2025
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓