Physics of planet trapping with applications to HL Tau

Author:

Cridland Alexander J12,Pudritz Ralph E23,Alessi Matthew2

Affiliation:

1. Leiden Observatory, Leiden University, NL-2300 RA Leiden, the Netherlands

2. Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4E8, Canada

3. Origins Institute, McMaster University, Hamilton, ON L8S 4E8, Canada

Abstract

ABSTRACT We explore planet formation in the HL Tau disc and possible origins of the prominent gaps and rings observed by ALMA. We investigate whether dust gaps are caused by dynamically trapped planetary embryos at the ice lines of abundant volatiles. The global properties of the HL Tau disc (total mass and size) at its current age are used to constrain an evolving analytic disc model describing its temperature and density profiles. By performing a detailed analysis of the planet–disc interaction for a planet near the water ice line including a rigorous treatment of the dust opacity, we confirm that water is sufficiently abundant (1.5 × 10−4 molecules per H) to trap planets at its ice line due to an opacity transition. When the abundance of water is reduced by 50 ${{\ \rm per\ cent}}$ planet trapping disappears. We extend our analysis to other planet traps: the heat transition, dead zone edge, and the CO2 ice line and find similar trapping. The formation of planets via planetesimal accretion is computed for dynamically trapped embryos at the water ice line, dead zone, and heat transition. The end products orbit in the inner disc (R < 3 au), unresolved by ALMA, with masses that range between sub-Earth to 5 Jupiter masses. While we find that the dust gaps correspond well with the radial positions of the CO2, CH4, and CO ice lines, the planetesimal accretion rates at these radii are too small to build large embryos within 1 Myr.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 12 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The Planet-forming Environment;Origins of Giant Planets, Volume 1;2021-12

2. Turbulent disc viscosity and the bifurcation of planet formation histories;Monthly Notices of the Royal Astronomical Society;2021-11-03

3. Molecules with ALMA at Planet-forming Scales (MAPS). XV. Tracing Protoplanetary Disk Structure within 20 au;The Astrophysical Journal Supplement Series;2021-11-01

4. Connecting planet formation and astrochemistry;Astronomy & Astrophysics;2020-10

5. Impact of vertical gas accretion on the carbon-to-oxygen ratio of gas giant atmospheres;Astronomy & Astrophysics;2020-03

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3