Orders of magnitude (magnetic moment)

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This page lists examples of magnetic moments produced by various sources, grouped by orders of magnitude. The magnetic moment of an object is an intrinsic property and does not change with distance, and thus can be used to measure "how strong" a magnet is. For example, Earth possesses an enormous magnetic moment, however we are very distant from its center and experience only a tiny magnetic flux density (measured in tesla) on its surface.

Contents

Knowing the magnetic moment of an object () and the distance from its centre () it is possible to calculate the magnetic flux density experienced on the surface () using the following approximation:

,

where is the constant of vacuum permeability.

Examples

Magnetic moment strength (from lower to higher orders of magnitude)
Factor (m 2A)ValueItem
10−459.0877×10−45 m2⋅A [1] Unit of magnetic moment in the Planck system of units.
10−274.3307346×10−27 m2⋅AMagnetic moment of a deuterium nucleus
10−261.4106067×10−26 m2⋅AMagnetic moment of a proton
10−249.284764×10−24 m2⋅AMagnetic moment of a positron
9.274…×10−24 m2⋅A Bohr magneton
10−180.65–2.65 nm2⋅A (1 nm2⋅A = 10−18 m2⋅A) [2] Magnetic moment of individual magnetite nanoparticles (20 nm diameter)
10-111.5×10−11 m2⋅A [3] Magnetic field of the human brain
3.75×10−11 m2⋅A [3]
10−57.99×10−5 m2⋅A [4] [5] NIST YIG (yttrium iron garnet) standard 1 mm sphere for calibrating magnetometers (SRM #2852)
10−48.6×10−4 m2⋅A [6] Needle in a thumbnail-sized compass
10−37.909×10−3 m2⋅A [7] Neodymium-iron-boron disc in a typical mobile phone
10-10.1 m2⋅A [8] Magnetic field of a typical refrigerator magnet
0.4824 m2⋅A [7] Neodymium-iron-boron (strongest grade) disc the same size as a US Penny
1001.17 m2⋅A [9] Neodymium-iron-boron N35 magnet of 1 cubic centimeter in volume
1.42 m2⋅A [9] Neodymium-iron-boron N52 magnet of 1 cubic centimeter in volume
1035.937×103 m2⋅A [7] A bowling ball made of neodymium-iron-boron (strongest grade)
1065×106 m2⋅A [10] Any magnet able to produce 1 tesla one metre away from its centre
10194×1019 m2⋅A [11] Magnetic field of Mercury
10201.32×1020 m2⋅A [11] Magnetic field of Ganymede
10226.4×1022 m2⋅A [12] Earth's magnetic field
10242.2×1024 m2⋅A [11] Magnetic field of Neptune
3.9×1024 m2⋅A [11] Magnetic field of Uranus
10254.6×1025 m2⋅A [11] Magnetic field of Saturn
10271.55×1027 m2⋅A [11] Magnetic field of Jupiter
10281×1028 m2⋅AMagnetic moment of a star or, equivalently, a white dwarf or a magnetar [13]
10291×1029 m2⋅A
10301×1030 m2⋅A [14]

Related Research Articles

<span class="mw-page-title-main">Magnetism</span> Class of physical phenomena

Magnetism is the class of physical attributes that occur through a magnetic field, which allows objects to attract or repel each other. Because both electric currents and magnetic moments of elementary particles give rise to a magnetic field, magnetism is one of two aspects of electromagnetism.

<span class="mw-page-title-main">Neutron star</span> Collapsed core of a massive star

A neutron star is the collapsed core of a massive supergiant star. It results from the supernova explosion of a massive star—combined with gravitational collapse—that compresses the core past white dwarf star density to that of atomic nuclei. Except for black holes, neutron stars are the smallest and densest known class of stellar objects. They have a radius on the order of 10 kilometers (6 mi) and a mass of about 1.4 M. Stars that collapse into neutron stars have a total mass of between 10 and 25 solar masses (M), or possibly more for those that are especially rich in elements heavier than hydrogen and helium.

<span class="mw-page-title-main">Magnetic field</span> Distribution of magnetic force

A magnetic field is a physical field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and to the magnetic field. A permanent magnet's magnetic field pulls on ferromagnetic materials such as iron, and attracts or repels other magnets. In addition, a nonuniform magnetic field exerts minuscule forces on "nonmagnetic" materials by three other magnetic effects: paramagnetism, diamagnetism, and antiferromagnetism, although these forces are usually so small they can only be detected by laboratory equipment. Magnetic fields surround magnetized materials, electric currents, and electric fields varying in time. Since both strength and direction of a magnetic field may vary with location, it is described mathematically by a function assigning a vector to each point of space, called a vector field.

<span class="mw-page-title-main">Magnetar</span> Type of neutron star with a strong magnetic field

A magnetar is a type of neutron star with an extremely powerful magnetic field (~109 to 1011 T, ~1013 to 1015 G). The magnetic-field decay powers the emission of high-energy electromagnetic radiation, particularly X-rays and gamma rays.

<span class="mw-page-title-main">Magnetic dipole</span> Magnetic analogue of the electric dipole

In electromagnetism, a magnetic dipole is the limit of either a closed loop of electric current or a pair of poles as the size of the source is reduced to zero while keeping the magnetic moment constant.

<span class="mw-page-title-main">Halbach array</span> Special arrangement of permanent magnets

A Halbach array is a special arrangement of permanent magnets that augments the magnetic field on one side of the array while cancelling the field to near zero on the other side. This is achieved by having a spatially rotating pattern of magnetisation.

<span class="mw-page-title-main">Magnetic moment</span> Magnetic strength and orientation of an object that produces a magnetic field

In electromagnetism, the magnetic moment or magnetic dipole moment is the combination of strength and orientation of a magnet or other object or system that exerts a magnetic field. The magnetic dipole moment of an object determines the magnitude of torque the object experiences in a given magnetic field. When the same magnetic field is applied, objects with larger magnetic moments experience larger torques. The strength of this torque depends not only on the magnitude of the magnetic moment but also on its orientation relative to the direction of the magnetic field. Its direction points from the south pole to north pole of the magnet.

<span class="mw-page-title-main">Pulsar</span> Rapidly rotating neutron star

A pulsar is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. This radiation can be observed only when a beam of emission is pointing toward Earth, and is responsible for the pulsed appearance of emission. Neutron stars are very dense and have short, regular rotational periods. This produces a very precise interval between pulses that ranges from milliseconds to seconds for an individual pulsar. Pulsars are one of the candidates for the source of ultra-high-energy cosmic rays.

In physics, the gyromagnetic ratio of a particle or system is the ratio of its magnetic moment to its angular momentum, and it is often denoted by the symbol γ, gamma. Its SI unit is the radian per second per tesla (rad⋅s−1⋅T−1) or, equivalently, the coulomb per kilogram (C⋅kg−1).

A quadrupole or quadrapole is one of a sequence of configurations of things like electric charge or current, or gravitational mass that can exist in ideal form, but it is usually just part of a multipole expansion of a more complex structure reflecting various orders of complexity.

In atomic physics, the electron magnetic moment, or more specifically the electron magnetic dipole moment, is the magnetic moment of an electron resulting from its intrinsic properties of spin and electric charge. The value of the electron magnetic moment is −9.2847646917(29)×10−24 J⋅T−1. In units of the Bohr magneton (μB), it is −1.00115965218059(13) μB, a value that was measured with a relative accuracy of 1.3×10−13.

A pulsar kick is the name of the phenomenon that often causes a neutron star to move with a different, usually substantially greater, velocity than its progenitor star. The cause of pulsar kicks is unknown, but many astrophysicists believe that it must be due to an asymmetry in the way a supernova explodes. If true, this would give information about the supernova mechanism.

<span class="mw-page-title-main">Radio-quiet neutron star</span> Neutron star that does not emit radio waves

A radio-quiet neutron star is a neutron star that does not seem to emit radio emissions, but is still visible to Earth through electromagnetic radiation at other parts of the spectrum, particularly X-rays and gamma rays.

A g-factor is a dimensionless quantity that characterizes the magnetic moment and angular momentum of an atom, a particle or the nucleus. It is the ratio of the magnetic moment of a particle to that expected of a classical particle of the same charge and angular momentum. In nuclear physics, the nuclear magneton replaces the classically expected magnetic moment in the definition. The two definitions coincide for the proton.

<span class="mw-page-title-main">Gauss's law for magnetism</span> Foundational law of classical magnetism

In physics, Gauss's law for magnetism is one of the four Maxwell's equations that underlie classical electrodynamics. It states that the magnetic field B has divergence equal to zero, in other words, that it is a solenoidal vector field. It is equivalent to the statement that magnetic monopoles do not exist. Rather than "magnetic charges", the basic entity for magnetism is the magnetic dipole.

This page lists examples of magnetic induction B in teslas and gauss produced by various sources, grouped by orders of magnitude.

<span class="mw-page-title-main">Gravitoelectromagnetism</span> Analogies between Maxwells and Einsteins field equations

Gravitoelectromagnetism, abbreviated GEM, refers to a set of formal analogies between the equations for electromagnetism and relativistic gravitation; specifically: between Maxwell's field equations and an approximation, valid under certain conditions, to the Einstein field equations for general relativity. Gravitomagnetism is a widely used term referring specifically to the kinetic effects of gravity, in analogy to the magnetic effects of moving electric charge. The most common version of GEM is valid only far from isolated sources, and for slowly moving test particles.

RRAT J1819-1458 is a Milky Way neutron star and the best studied of the class of rotating radio transients (RRATs) first discovered in 2006.

Magnets exert forces and torques on each other through the interaction of their magnetic fields. The forces of attraction and repulsion are a result of these interactions. The magnetic field of each magnet is due to microscopic currents of electrically charged electrons orbiting nuclei and the intrinsic magnetism of fundamental particles that make up the material. Both of these are modeled quite well as tiny loops of current called magnetic dipoles that produce their own magnetic field and are affected by external magnetic fields. The most elementary force between magnets is the magnetic dipole–dipole interaction. If all magnetic dipoles for each magnet are known then the net force on both magnets can be determined by summing all the interactions between the dipoles of the first magnet and the dipoles of the second magnet.

In physics, the Euler–Heisenberg Lagrangian describes the non-linear dynamics of electromagnetic fields in vacuum. It was first obtained by Werner Heisenberg and Hans Heinrich Euler in 1936. By treating the vacuum as a medium, it predicts rates of quantum electrodynamics (QED) light interaction processes.

References

  1. That is,
  2. Sievers, Sibylle; Braun, Kai-Felix; Eberbeck, Dietmar; Gustafsson, Stefan; Olsson, Eva; Schumacher, Hans Werner; Siegner, Uwe (2012-09-10). "Quantitative Measurement of the Magnetic Moment of Individual Magnetic Nanoparticles by Magnetic Force Microscopy". Small . 8 (17): 2675–2679. doi:10.1002/smll.201200420. PMC   3561699 . PMID   22730177.
  3. 1 2 Gilder, Stuart A.; Wack, Michael; Kaub, Leon; Roud, Sophie C.; Petersen, Nikolai; Heinsen, Helmut; Hillenbrand, Peter; Milz, Stefan; Schmitz, Christoph (2018). "Distribution of magnetic remanence carriers in the human brain". Scientific Reports. 8 (11363): 11363. doi:10.1038/s41598-018-29766-z. PMC   6063936 . PMID   30054530.
  4. Erdevig, Hannah E.; Russek, Stephen E.; Carnicka, Slavka; Stupic, Karl F.; Keenan, Kathryn E. (May 2017). "Accuracy of magnetic resonance based susceptibility measurements". AIP Advances . 7 (5). doi:10.1063/1.4975700. The SQUID magnetometer is calibrated with a NIST YIG (yttrium iron garnet) sphere standard reference material (SRM #2852) whose room temperature moment is (79.9 ± 0.3) × 10−6 A·m2
  5. Handwerker, Carol A.; John, Rumble (2002-05-20). "Certificate of Analysis – Standard Reference Material® 2853 – Magnetic Moment Standard - Yttrium Iron Garnet Sphere" (PDF). National Institute of Standards and Technology . Retrieved 2024-08-13. SRM 2853 consists of a yttrium iron garnet (YIG) sphere with a nominal diameter of 1 mm and a nominal mass 2.8 mg. The certified value for the specific magnetization, σ, at 298 K in an applied magnetic field of 398 kA/m (5000 Oe) is: σ = 27.6 A·m2/kg ± 0.1 A·m2/kg (27.6 emu/g ± 0.1 emu/g).
  6. Cookson, Esther; Nelson, David; Michael, Anderson; McKinney, Daniel L.; Barsukov, Igor (2019). "Exploring Magnetic Resonance with a Compass". Phys. Teach. 57 (9): 633–635. arXiv: 1810.11141 . doi:10.1119/1.5135797 . Retrieved 2024-08-09. For a thumbnail-sized compass, we (empirically) estimate the magnetic moment to 0.86×10−3 A⋅m2 and the moment of inertia to 1.03×10−11 kg⋅m2.
  7. 1 2 3 "What is the MAGNETIC MOMENT?". Adams Magnetic. 6 August 2021. Retrieved 2024-07-24.
  8. Tal, Assaf (2021). "Imaging the Brain using MRI: From Physics to Applications – Lecture 3, Spin Dynamics" (PDF). Weizmann Institute Of Science. Retrieved 2024-08-09. A typical refrigerator magnet might have a macroscopic magnetic moment of about 0.1 J/T.
  9. 1 2 Stanford Magnets (2024-06-03). "Magnetization Features: Magnetic Moment, Dipole, and Models" . Retrieved 2024-08-12.
  10. This is a consequence of the definition of the magnetic constant.
  11. 1 2 3 4 5 6 Durand-Manterola, Hector Javier (2010-07-26). "Dipolar Magnetic Moment of the Bodies of the Solar System and the Hot Jupiters". arXiv: 1007.4497 [astro-ph.EP].
  12. "Earth's Magnetic Field". Harvard University. Retrieved 2024-07-24.
  13. Magnetars have enormous magnetic flux densities on their surfaces due to the small radius, however the total magnetic field of the original star does not increase during the collapse, but actually decreases with time. Cf. Reisenegger, A. (2003). "Origin and Evolution of Neutron Star Magnetic Fields". arXiv: astro-ph/0307133 . Generally speaking, young neutron stars appear to have strong magnetic fields ∼1011−15 G ('classical' radio pulsars, 'magnetars', X-ray pulsars), whereas old neutron stars have weak fields ≲ 109 G (ms pulsars, lowmass X-ray binaries). If these two groups have an evolutionary connection, their dipole moment must decay. Millisecond pulsars are believed to have been spun up to their fast rotation by accretion from a binary companion, a remnant of which is in most cases still present (e.g., Phinney & Kulkarni 1994). The reduction in the magnetic dipole moment may be a direct or indirect consequence of the accretion process, or just an effect of age.
  14. Toropina, O. D.; Romanova, M. M.; Lovelace, R. V. E. (2006). "Spinning-down of moving magnetars in the propeller regime". Monthly Notices of the Royal Astronomical Society. 371 (2): 569–576. arXiv: astro-ph/0606254 . doi: 10.1111/j.1365-2966.2006.10667.x .

See also