Wei Zhu(祝伟)
I'm now an Assistant Professor in the Department of Astronomy at Tsinghua University in Beijing.
Wei Zhu (祝伟)
2021年全国行星科学大会,苏州
2021-06-20
(Slides accessible here)
Image credit: iLectureOnline
Giant planet formation (\(\lesssim\) 10 Myr)
Terrestrial planet formation (\(\sim\) 100 Myr)
Transit (ground)
Transit (space)
Radial velocity
Microlensing
Imaging
Hot Jupiters
Cold Jupiters
Super Earths
Cold Neptunes
What You See Is Not What You Get!
Based on data from NASA Exoplanet Archive.
Zhu & Dong (2021, ARAA)
(see also Fressin et al. 2013, Petigura et al. 2018, Hsu et al. 2019, etc)
(Colors mean different observed multiplicities.)
(How are planets in the same system distributed?)
Figures from Winn & Fabrycky (2015) and Zhu & Dong (2021)
Cold Jupiters
Cold Jupiters
Super Earths
22 from Kepler (triangles) + 39 from RV (squares)
\( P({\rm SE}|{\rm CJ}) \cdot P({\rm CJ}) = P({\rm CJ}|{\rm SE}) \cdot P({\rm SE}) \) \( \rightarrow P({\rm SE}|{\rm CJ})=100\% \)
\(P({\rm CJ}|{\rm SE}) \approx 33\% {\rm ~vs.~} P({\rm CJ})=10\%\)
(see also Batygin & Laughlin 2015)
Cold Jupiters
Cold Neptunes
Paczynski (1986); Mao & Paczynski (1991)
\(t_{\rm E} \sim 30{\rm days} \left(\frac{M_{\rm L}}{M_\odot}\right)^{1/2} \)
\( t_q \sim 40{\rm min} \left(\frac{q}{10^{-6}}\right)^{1/2} \left( \frac{t_{\rm E}}{30 \rm days}\right) \)
背景恒星亮度
背景恒星
”透镜“星体
\( t_{\rm E} \)
\( t_q \)
银河系中心
1 deg
银河系中心
1 deg
Neptune
Jupiter
臧伟呈
杨弘靖
“流浪” = 距离主星距离超过~15 AU
银河系中可能存在与恒星数目相当的流浪行星 (KMTNet+OGLE约1例/年)
Mroz et al. (2017, 2021)
a Mars-mass FFP!
3'
9"
Images from Pietrukowicz et al. (2019)
Figure from Mao (2012)
Small-size stars
Intermediate-size stars
Large-size stars
Time in event unit
Magnification in brightness (log)
Figure from Penny et al. (2019)
See talk on ET by 张辉
Many (or majority) of them reside in multi-planet systems.
Dynamical interactions between planets may have largely reshaped the system architecture.
(Slides accessible here)
Kepler mission (2009-2018):
Ongoing/Future transit missions:
Gaia astrometry:
Microlensing:
EarthTwo?
TESS
Cheops
2009
2025
2020
2018
2015
2012
Kepler
Gaia
LAMOST
KMTNet
Dedicated RV telescope?
WFIRST
(+CSST)
Transit singles have \(\sigma_e\approx0.3\), whereas transit multis have \(\sigma_e\approx0.05\) (Van Eylen et al. 2015, 2019, Xie et al. 2016, Mills et al. 2019).
Transit duration \(T\)
Zhu & Dong (2021)
Systems with more planets have smaller eccentricities and are dynamically colder.
Transit singles
Transit doubles
Transit triples
Transit quadruples
Spacing in mutual Hill radii
By Wei Zhu(祝伟)
A presentation in the 2021 National Conference on Planetary Science in Suzhou.
I'm now an Assistant Professor in the Department of Astronomy at Tsinghua University in Beijing.