Songhu Wang
Physics and Astronomy · Indiana University
Publications
132
Citations
2,320
Est. group size
—
Recurring co-author estimate
Active years
24
Publishing since 2003
Songhu Wang studies exoplanets — planets orbiting stars other than our Sun — with a focus on how giant planets like hot and warm Jupiters form and evolve. Much of the work measures the alignment between planets' orbits and their host stars' spin, and explores how a star's chemical makeup (such as being metal-rich) relates to the architecture of its planetary system. The research combines radial-velocity and photometric observations, often using NASA's TESS mission data.
Publication activity has grown over the last decade, rising from around 5 per year in 2017 to a peak in 2023, and remaining consistently high (about 14 per year on average over the last five years).
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- Unified Formation Channel of Hot and Warm Jupiters via Planet–Planet Scattering
The Astrophysical Journal Letters · 2026
- TOI-778 TESS radial velocity & optical photometry
Strasbourg Astronomical Data Center · 2026
- HIRES TOI-1136s planets and planet b radial velocities
Strasbourg Astronomical Data Center · 2026
- The origin and tidal evolution of hot Jupiters constrained by a broken age–frequency relation
Nature Astronomy · 2025
- Plastidic glutamine synthetase (GS2) enhances nitrogen assimilation and protein production in duckweed using urea nitrogen source
International Journal of Biological Macromolecules · 2025
- Migration and Evolution of giant ExoPlanets (MEEP). II. Super-Jupiters and Lithium-rich host stars
Monthly Notices of the Royal Astronomical Society · 2025
- Short-period Small Planets with High Mutual Inclinations are More Common around Metal-rich Stars
The Astrophysical Journal Letters · 2025
- Short-Period Small Planets with High Mutual Inclinations are more Common around Metal-Rich Stars
arXiv (Cornell University) · 2025
- Statistical Reevaluation of the Ultra-short-period Planet Classification Boundary: Smaller Planets within 1 Day, Larger Period Ratios below 2 Days
The Astronomical Journal · 2025
- Statistical Reevaluation of the USP Classification Boundary: Smaller Planets Within 1 Day, Larger Period Ratios Below 2 Days
arXiv (Cornell University) · 2025
- From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest <i>M</i> <sub> <i>p</i> </sub>/<i>M</i> <sub>*</sub> Systems Exhibit Low Obliquities, Even around Hot Stars*
The Astrophysical Journal Letters · 2025
- TOI-880 is an Aligned, Coplanar, Multiplanet System
The Astronomical Journal · 2025
- Earths Are Not Super-Earths, Saturns Are Not Jupiters: Imprints of Pressure-bump Planet Formation on Planetary Architectures
The Astrophysical Journal Letters · 2024
- A Larger Sample Confirms Small Planets around Hot Stars Are Misaligned <sup>∗</sup>
The Astrophysical Journal Letters · 2024
- Origins of Super Jupiters: TOI-2145b has a Moderately Eccentric and Nearly Aligned Orbit
The Astronomical Journal · 2024
- arXiv (Cornell University)×35
- The Astronomical Journal×29
- The Astrophysical Journal Letters×15
- Monthly Notices of the Royal Astronomical Society×5
- Astronomy and Astrophysics×4
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
Claim or correct this profile