39 citations
- Meteorological Research Institute17 papers
- Kobe UniversityJP7 papers
- Kyoto UniversityJP6 papers
- National Astronomical Observatory of JapanJP6 papers
- The University of TokyoJP5 papers
- Tohoku UniversityJP5 papers
- Kyoto Sangyo UniversityJP4 papers
- Japan Spaceguard AssociationJP3 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP3 papers
- Konan UniversityJP3 papers
- Kyushu UniversityJP3 papers
- RIKEN Center for Computational ScienceJP3 papers
5 papers · 1 filter
Relative abundances of CO2, CO, and CH4 in atmospheres of Earth-like lifeless planets
Yasuto Watanabe, Kazumi Ozaki
Carbon is an essential element for life on Earth, and the relative abundances of major carbon species (CO2, CO, and CH4) in the atmosphere exert fundamental controls on planetary c…
Modification of the Shower Database of the IAU Meteor Data Center
M. Hajdukova, R. Rudawska, T. J. Jopek +3
The Shower Database (SD) of the Meteor Data Center (MDC) has been operating for 15 years and is used by the entire community of meteor astronomers. It contains meteor showers categ…
Relationship between Radar Cross Section and Optical Magnitude based on Radar and Optical Simultaneous Observations of Faint Meteors
Ryou Ohsawa, Akira Hirota, Kohei Morita +40
Radar and optical simultaneous observations of meteors are important to understand the size distribution of the interplanetary dust. However, faint meteors detected by high power l…
New constraint on the atmosphere of (50000) Quaoar from a stellar occultation
Ko Arimatsu, Ryou Ohsawa, George L. Hashimoto +35
We report observations of a stellar occultation by the classical Kuiper belt object (50000) Quaoar occurred on 28 June 2019. A single-chord high-cadence (2 Hz) photometry dataset w…
A Fireball and Potentially Hazardous Binary Near-Earth Asteroid (164121) 2003 YT
Toshihiro Kasuga, Mikiya Sato, Masayoshi Ueda +3
We present a fireball detected in the night sky over Kyoto, Japan on UT 2017 April 28 at by the SonotaCo Network. The absolute visual magnitude is $M…