Jupiter – Détails, épisodes et analyse
Détails du podcast
Informations techniques et générales issues du flux RSS du podcast.


Stay informed about the newest discoveries, scientific missions, and technological advancements that help us understand Jupiter's complex atmosphere and magnetic field. Whether you're a space enthusiast or a curious learner, "Planet Jupiter" offers a captivating and educational experience. Subscribe now and embark on a journey to explore the wonders of Jupiter.
FOr more info https://www.quietperiodplease.com/
Classements récents
Dernières positions dans les classements Apple Podcasts et Spotify.
Apple Podcasts
🇬🇧 Grande Bretagne - astronomy
15/05/2026#98🇬🇧 Grande Bretagne - astronomy
14/05/2026#92🇩🇪 Allemagne - astronomy
27/04/2026#100🇬🇧 Grande Bretagne - astronomy
26/04/2026#97🇩🇪 Allemagne - astronomy
26/04/2026#94🇬🇧 Grande Bretagne - astronomy
25/04/2026#87🇩🇪 Allemagne - astronomy
25/04/2026#92🇬🇧 Grande Bretagne - astronomy
24/04/2026#85🇩🇪 Allemagne - astronomy
24/04/2026#85🇬🇧 Grande Bretagne - astronomy
23/04/2026#75
Spotify
Aucun classement récent disponible
Liens partagés entre épisodes et podcasts
Liens présents dans les descriptions d'épisodes et autres podcasts les utilisant également.
See all- https://www.quietperiodplease.com/
3680 partages
Qualité et score du flux RSS
Évaluation technique de la qualité et de la structure du flux RSS.
See allScore global : 64%
Historique des publications
Répartition mensuelle des publications d'épisodes au fil des années.
Planet Jupiter Destiny of a Cosmic Monarch
lundi 17 juin 2024 • Durée 21:36
- Size: Jupiter has a diameter of about 142,984 kilometers (88,846 miles), making it more than 11 times the diameter of Earth. It is so massive that it could fit all the other planets in the solar system inside it.
- Mass: It has a mass of 1.898 × 10^27 kilograms, which is approximately 318 times the mass of Earth.
- Orbit and Rotation: Jupiter orbits the Sun at an average distance of 778 million kilometers (484 million miles). It takes about 12 Earth years to complete one orbit around the Sun. However, a day on Jupiter (one full rotation) is only about 10 hours long, making it the fastest rotating planet in the solar system.
- Atmosphere: Jupiter’s atmosphere is composed primarily of hydrogen (about 90%) and helium (about 10%), with trace amounts of other gases such as methane, ammonia, and water vapor. The atmosphere features multicolored bands, created by strong winds and chemical reactions at different altitudes.
- Great Red Spot: One of Jupiter's most famous features is the Great Red Spot, a gigantic storm that has been raging for at least 400 years. This anticyclonic storm is larger than Earth and is characterized by its reddish hue, which is still not fully understood.
- Magnetic Field: Jupiter has a powerful magnetic field, about 20,000 times stronger than Earth’s. This magnetic field creates intense radiation belts and influences the planet’s many moons.
- Moons: Jupiter has at least 79 known moons, with the four largest being the Galilean moons: Io, Europa, Ganymede, and Callisto. These moons are some of the most interesting objects in the solar system, with features such as active volcanism (Io), subsurface oceans (Europa), and diverse geological landscapes (Ganymede and Callisto).
- Space Missions:
- Pioneer 10 and Pioneer 11 were the first spacecraft to visit Jupiter in the early 1970s.
- Voyager 1 and Voyager 2 provided detailed images and data about the planet and its moons in 1979.
- Galileo orbited Jupiter from 1995 to 2003, offering extensive data on the planet and its moons.
- Juno, launched in 2011, is currently in orbit around Jupiter, studying its atmosphere, magnetic field, and internal structure.
- Radiation Belts: Jupiter's intense magnetic field creates radiation belts that are so powerful they can damage spacecraft electronics.
- Ring System: While not as prominent as Saturn's, Jupiter has a faint ring system composed mainly of dust particles ejected from its moons.
- Auroras: Jupiter’s poles exhibit spectacular auroras, caused by interactions between the planet’s magnetic field and charged particles from the solar wind.









