Photometric Analysis of Asteroids in the Phocaea Region
The Phocaea asteroid family, one of the large ancient families located in the inner main belt, may be the sources of near-Earth asteroids (NEAs) due to the nearby 3:1 mean motion resonance with Jupiter, the ν 6 secular resonance, and the Yarkovsky and Yarkovsky–O'Keefe–Radzievskii–Paddack (YORP...
Saved in:
| Main Authors: | Xiaoyun Xu, Xiaobing Wang, Karri Muinonen, Shenghong Gu, Antti Penttilä, Fukun Xu, Leilei Sun, Jing Huang, Pengfei Zhang, Ao Wang |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astronomical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-3881/add3f4 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Insights on the Rotational State and Shape of Asteroid (203) Pompeja from TESS Photometry
by: Oriel A. Humes, et al.
Published: (2024-01-01) -
Long-term Spectral Monitoring of Active Asteroid (6478) Gault: Implications for the H Chondrite Parent Body
by: Adam Battle, et al.
Published: (2025-01-01) -
Rare Phosphides and Nitrides in Igneous Clasts within Aqueously Altered Chondrites
by: Lucas. R. Smith, et al.
Published: (2025-01-01) -
Development of a technique to identify μm-sized organic matter in asteroidal material: An approach using machine learning
by: Rahul Kumar, et al.
Published: (2025-09-01) -
Galaxy Spectroscopy without Spectra: Galaxy Properties from Photometric Images with Conditional Diffusion Models
by: Lars Doorenbos, et al.
Published: (2024-01-01)