Please watch this video first. Seven small dots rotating at various speeds around a large orange dot make a sound each time they go around a circle. The pitch of the rhythmically played notes differs from point to point, and unique chords are played depending on the combination of points with the right timing.
【▲ 動画:The Sounds of a New Planetary System (NASA Data Sonification)】
(Credit: Bishop’s University /Jason Rowe)
This video, which seems like a kind of art, depicts exoplanets (including candidates) orbiting the star Kepler-385, located approximately 4,670 light years away in the constellation Cygnus. ) was created using the sonification
method. Kepler-385 is a star that is approximately 10% larger in diameter and has a surface temperature approximately 5% higher than the Sun.
*…A method of conveying information such as images using nonverbal sounds. Also known as audible.
[▲ An imaginary drawing of an extrasolar planet orbiting the star “Kepler 385” (Credit: NASA/Daniel Rutter)]
[▲ Image diagram showing the orbits of seven exoplanets orbiting the star “Kepler 385” (Credit: NASA/Daniel Rutter)]
According to a research team led by Jack Lissauer of the Ames Research Center, the orbital period of the seven planets is about 86 days for the outermost planet, and only about 0.6 days for the innermost planet. In other words, the seven planets are orbiting very close to Kepler-385. Comparing the energy per unit area incident on the planets, each planet in Kepler 385 receives more energy than any other planet in the solar system, which NASA describes as “hot as hell.” Masu. A paper summarizing the results of the research team that reexamined Kepler’s observational data will be published in The Journal of Planetary Science, and a preprint is available on arXiv.
Source NASA– Scorching, Seven-Planet System Revealed by New Kepler Exoplanet List Bishop’s University– New Kepler Exoplanet Catalogue Reveals Exoplanet Architectures and Multiplanet System Lissauer et al.
– Updated Catalog of Kepler Planet Candidates: Focus on Accuracy and Orbital Periods (arXiv)
Text/sorae editorial department