Galileo
Jupiter's magnetic field is caused by the convection of liquid metallic hydrogen in its outer core. This creates electric currents that produce the magnetic field. Jupiter's rapid rotation also plays a role in generating its strong magnetic field.
Magnetic domains.
Mars does not have a global magnetic field, but it does have localized regions of magnetic fields. The tilt of these magnetic fields varies across different regions on Mars, ranging from about 0 to 180 degrees.
One common method is using a magnetic field sensor and mapping the magnetic field strength around the magnet. By observing the variations in the field strength, you can identify two distinct regions where the magnetic field is concentrated. Another approach is using iron filings to visually show the magnetic field lines around the magnet, which can help visualize the two regions of concentrated magnetic strength.
The moon does not have a global magnetic field like Earth. However, there are localized regions on the moon's surface that have magnetic properties, likely due to past interactions with Earth's magnetic field when the moon was forming.
The Juno spacecraft collected data about Jupiter's magnetic field and polar regions. Juno arrived at Jupiter in July 2016 and orbits the planet to study its atmosphere, magnetosphere, and interior structure.
Jupiter's magnetic field is caused by the convection of liquid metallic hydrogen in its outer core. This creates electric currents that produce the magnetic field. Jupiter's rapid rotation also plays a role in generating its strong magnetic field.
They are called "domains. The collected domains form the "north" and "south" poles of a magnet, and create a magnetic field (with a magnetic flux) around the collection of atoms.
They are called "domains. The collected domains form the "north" and "south" poles of a magnet, and create a magnetic field (with a magnetic flux) around the collection of atoms.
Magnetic domains.
Jupiters gravitational field strength is 25 Nkg^-1
domains
The neutral point of a magnetic field is the point in space where the magnetic field intensity is zero. At this point, the magnetic forces acting on a particle will cancel each other out, resulting in no net force. This occurs in regions where magnetic field lines from opposite directions meet and cancel each other.
Mars does not have a global magnetic field, but it does have localized regions of magnetic fields. The tilt of these magnetic fields varies across different regions on Mars, ranging from about 0 to 180 degrees.
The shape of a magnet can impact its magnetic field by influencing the distribution and direction of the magnetic field lines. For example, a bar magnet will have a magnetic field that extends from one pole to the other, while a horseshoe magnet will concentrate the field between its poles. The shape can also affect the strength and direction of the magnetic field in different regions.
One common method is using a magnetic field sensor and mapping the magnetic field strength around the magnet. By observing the variations in the field strength, you can identify two distinct regions where the magnetic field is concentrated. Another approach is using iron filings to visually show the magnetic field lines around the magnet, which can help visualize the two regions of concentrated magnetic strength.
A magnetic needle kept in uniform magnetic field will experience zero net force but non-zero net torque........Since the magnetic lines are uniform,the force acting on each end of the needlewill be equal and opposite.So it will cancel each other resulting zero net force.