Jupiter and the Jovian Planets Formation of Jovian
- Slides: 42
Jupiter and the Jovian Planets
Formation of Jovian Planets • Step 1 Accretion of planetesimals to form large Earth-like solid planet cores of rocks, iron, nickel • Masses of Cores in terms of Earth’s mass Jupiter 28 Saturn 17 Uranus 3. 5 Neptune 4. 3 • Step 2 Lighter gases condense on to the planet cores due to gravity and cold temperatures
Jupiter – Formation of Planetary Systems
Jupiter – “A Failed Star” • Jupiter is 318 times more massive than the Earth; yet, it is 80 times too small to become a star, i. e. make nuclear energy from fusion like the Sun • But Jupiter (and Saturn) emits roughly twice the energy it receives from the Sun • Energy derives from self-gravity gravitational compression of the interior (Jupiter shrinks about an inch per century) • Surface T = 124 K, but expected 109 K (assuming Sun to be the only source) • Jupiter radiates (124 / 109)4 = 1. 7 times more energy than would be expected
Jupiter Interior Molecular Hydrogen Metallic Hydrogen “Ice” Rock
Conditions inside Jupiter • Composition like the Sun: mostly H, He • Atmosphere 500 miles thick, largely H 2, He, and CH 4, NH 3, H 2 O • Very low mean density of 1. 33 g/cc (including compressed core) planet must be largely liquid • “Surface” is largely top of liquid hydrogen ocean (Jovian planets have no solid surface), where “Air pressure” is 500 x Earth’s, and temperature of 4000 F • Equator and poles do not rotate at same rate (oblate shape): 9 h 50 min and 9 h 55 min respectively • Huge magnetic field, why?
Jupiter’s Interior • Most of Jupiter is about 40, 000 mile deep ocean of liquid hydrogen • But it is mostly metallic H 2: high density and pressure compress the H 2 molecule so that they “share” electrons, i. e. electrons can move around like in a metal conduct electricity • “Core” is solid ice, rock, iron, nickel at very high pressure (1 billion lbs / sq. inch) - core itself is about 28 x Earth’s mass - temperature 50, 000 F
Saturn Interior Molecular Hydrogen Metallic Hydrogen “Ice” Rock
Interiors of Jupiter and Saturn
Interiors of Uranus & Neptune Molecular Hydrogen Rocky Cores Slushy “Ice”Mantles Uranus Neptune
Jupiter Saturn Metallic Hydrogen Uranus Neptune Earth Jupiter and Saturn have metallic hydrogen mantle; Uranus and Neptune don’t
Temperature (pressure) in Jupiter rises faster than in Saturn with depth Although T and P are high in the cores, not sufficient for nuclear fusion like stars Require millions of degrees!
Jupiter – The King of Planets Stripes, What are they?
The Red Spot – What is it? First seen by Galileo, over 350 years ago ! Twice the size of the Earth
A long lasting (over 300 years!!), internally powered, cyclonic storm (but what sustains it? )
Rapid rotation of Jupiter Period ~ 10 hrs In spite of its size (318 times more massive than the Earth) it rotates 2 ½ times faster. But there is very little tilt of rotation axis (3 degrees) No Seasons !
Internal energy source Strong convection currents What provides the internal energy source ? Self-gravity!
Jupiter – Vital Statistics • Equatorial radius = 71, 500 Kms • Orbital period = 11. 86 Earth years • Mean density = 1. 33 g/cc (3. 5 times lower than Earth’s) • Indicates mostly H 2 interior, but at tremendous pressure Metallic Hydrogen (conducts electricity!), up to about 20, 000 Kms into the center • Alternating lighter and darker stripes on the surface are zones of rising (warmer) and falling (cooler) material
Vertical Convection: “Belts” and “Zones” Cloud patterns are at different temperatures (altitudes) and wind speeds; tremendous “wind shear” (reverse direction at different altitudes)
Jovian Interior Mostly metallic hydrogen electrically conducting interior huge magnetic field
Jovian Magnetosphere Note that scale on bottom right! Jupiter’s magnetic field is 20, 000 times stronger than Earth’s
Jupiter’s Magnetic Field • 20, 000 times stronger than Earth’s, due to convection in liquid metallic H 2 interior; convection is due to rapid rotation • “Fast electrons” produced when the solar wind hits Jupiter’s magnetosphere • Lethal rays: density of particles is thousands of times fatal human dosage • Magnetosphere extends up to Saturn, 5 AU away
Jupiter and the 4 Galilean Moons: Io, Europa, Ganymede, Callisto
Relative sizes of Galilean Moons
Galilean Moons: Io, Europa, Ganymede, Callisto Rocky to Icy (Ganymede is the largest moon in the solar system) Io and Europa are mostly rocky but Ganymede and Callisto have more ices; Densities: 3. 6, 3. 0, 1. 9, 1. 8 g/cc respectively.
Jovian Moons • In addition to the 4 Galilean satellites, 12 other moons of Jupiter have been discovered • Owing to Jupiter’s tidal effects all Galilean moons are ‘synchronous rotators’: they keep the same face towards Jupiter • Voyager also found a ring around Jupiter, in between two small moons before Io • Latest NASA probe of Jupiter is called Galileo
IO • Closest large moon to Jupiter • Orbital period = 42 hrs • Surface has no impact craters, so less than 1 million years old • Many volcanic craters – active volcanoes • No water (too hot), but lots of sulfur on surface (sulfur condenses easily; appears black when heated)
Erupting volcanoes (taped live!)
Hot-spots at volcanoes
Io’s Volcanic Activity • Eight volcanoes seen by Voyager (many more seen since) • Plumes rise 100 miles, spread over hundreds of miles • Surface temp roughly 700 F near volcanoes, -250 F away from them • Caused by Jupiter’s tidal effect large land tides, up to 100 yards in height • Friction inside Io produces heat and volcanic activity (“squeezed” like a ketchup bottle !)
Pizza?
Volcanic features on Io
Typical volcanic feature on Io
Io’s orbit around Jupiter: Sulfur emission (spectral lines)
Io and Jupiter’s Magnetic Field • Magnetic field rotates with the planet, and electrifies the orbit of IO plasma (charged particles) torus surrounding orbit of IO; contains Sulfur ions S+ (emission spectral lines detected on the Earth)
Electrically charged atmosphere surrounding Jupiter and orbit of Io
Radio emission from around Jupiter - “Synchrotron radiation” at radio wavelengths is produced by “fast electrons” from the magnetosphere - Jupiter’s radio signals are detected on the earth! Interfere with radio Communications with CB, short-wave radio, radar, UHF TV, etc.
Europa: Ice rafts moving on liquid water oceans Very thin Oxygen atmosphere has been detected on Europa
Comparison of Jovian Moons: Evolution due to Jupiter’s gravity Resolution Rocky Icy
Sizes and Distances of Galilean Satellites Sizes relative to Earth’s Moon ( = 1): 1. 1, 0. 9, 1. 5, 1. 4 respectively
Many moons of Jupiter
- Are jovian planets more dense than terrestrial
- Jupiter is noticeably oblate because
- Why do jovian planets have rings
- Why do jovian planets have rings
- Jupiter magnetosphere
- The two outer jovian planets appear bluish in color because
- What separates inner and outer planets
- The inner solar system by leslie
- Inner terrestrial planets
- The first four outer planets do not have solid
- Formation initiale vs formation continue
- Romeo and juliet globe theatre
- Mars jupiter and saturn show retrograde motion because
- Mars, jupiter, and saturn show retrograde motion because
- Neptune jovian
- Jovian
- Jovian planet
- Jovian gas giant
- What is the 2nd smallest planet in our solar system
- What separates the inner and outer planets
- The heavens themselves the planets and this centre
- My very excited mother just served us nachos
- Andor planet
- Hình ảnh bộ gõ cơ thể búng tay
- Slidetodoc
- Bổ thể
- Tỉ lệ cơ thể trẻ em
- Voi kéo gỗ như thế nào
- Thang điểm glasgow
- Hát lên người ơi
- Các môn thể thao bắt đầu bằng từ đua
- Thế nào là hệ số cao nhất
- Các châu lục và đại dương trên thế giới
- Công của trọng lực
- Trời xanh đây là của chúng ta thể thơ
- Cách giải mật thư tọa độ
- 101012 bằng
- độ dài liên kết
- Các châu lục và đại dương trên thế giới
- Thể thơ truyền thống
- Quá trình desamine hóa có thể tạo ra
- Một số thể thơ truyền thống
- Cái miệng nó xinh thế chỉ nói điều hay thôi