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Jupiter has the strongest mean equatorial field and the largest magnetic dipole moment of these three planets in NASA Goddard’s like-for-like comparison. Saturn shows why the metric matters: its dipole moment is about 600 times Earth’s, yet its listed mean equatorial field is weaker than Earth’s. The planets also differ in what powers their dynamos, how their magnetic axes align with their spin axes, and how their moons and surrounding plasma shape their magnetospheres.

The short answer to “Is Jupiter’s magnetic field stronger than Earth’s?” is yes on the specific measures in that comparison: Jupiter’s mean equatorial field is about 14 times Earth’s, and its dipole moment is about 20,000 times Earth’s. But a field-strength ratio, a dipole-moment ratio, and a magnetosphere’s dimensions describe different things. Saturn makes that distinction especially clear.

At a glance

Planet Mean equatorial field Dipole moment (Earth = 1) Dipole-axis tilt from spin axis Approximate rotation period
Earth 0.31 gauss 1 About 11.3° 24 hours
Jupiter 4.28 gauss About 20,000 About 9.6° 9.9 hours
Saturn 0.22 gauss About 600 About 0° 10.7 hours

All values in this table come from NASA Goddard Space Flight Center’s 2002 comparison, which attributes the figures to Bagenal (1992). The table is useful because it compares the planets within one consistent frame; later observations, models, locations, and definitions can produce different values. NASA Goddard’s planetary magnetic-field comparison.

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Read each row as a separate comparison, not as one overall score. Mean equatorial field is a field-strength figure for a stated region and metric. Dipole moment is a measure of the large-scale magnetic source. Axis tilt describes geometry, and rotation period gives a sense of how quickly each planet spins. None of those entries by itself tells you the full size or behavior of a magnetosphere.

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What do “field strength,” “dipole moment,” and “magnetosphere” mean?

They describe related but different parts of a planet’s magnetic environment. A number for one should not be treated as a substitute for another: local field strength describes the field at a specified place, dipole moment describes the large-scale magnetic source, and magnetosphere size describes the region influenced by that field and its surrounding plasma.

Field strength: a measurement at a location

Field strength is meaningful only with a location and a stated metric. The table above uses mean equatorial field, measured in gauss: on that basis, Jupiter’s listed value of 4.28 gauss is about 14 times Earth’s 0.31 gauss, while Saturn’s 0.22 gauss is lower than Earth’s. This is not a claim that the field has the same strength everywhere around each planet.

The word “mean” matters, too: the table is not giving a universal surface value that applies at every latitude or location. A field varies across a planet’s magnetic environment. So when comparing numbers, check what the number measures and where the comparison applies. The figures in the table are a useful, internally consistent historical frame, not a promise that every mission or model will report an identical value.

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Different comparison bases help explain why NASA pages may give ratios that do not match the table’s roughly 14-to-1 Jupiter-to-Earth equatorial comparison. NASA’s Jupiter facts page describes Jupiter’s magnetic field more broadly as 16–54 times Earth’s, but that range is not presented as the same equatorial-field metric. NASA’s Saturn facts page says Saturn’s field is 578 times Earth’s, without establishing on that page that it is a like-for-like equatorial comparison. These figures should be quoted with their source and basis, not blended into a single ranking. NASA’s Jupiter facts page and NASA’s Saturn facts page.

Dipole moment: the scale of the large-scale source

Dipole moment is a different way to compare a planet’s overall magnetic source. In NASA Goddard’s table, Earth is set to 1, Jupiter is about 20,000 Earth units, and Saturn is about 600. Thus Saturn’s dipole moment is much larger than Earth’s even though its listed mean equatorial field is weaker. There is no contradiction: one figure compares the large-scale source, while the other is a field value for a specified region and metric.

This distinction answers the natural question, “Why can Saturn have a larger magnetic moment than Earth but a weaker listed equatorial field?” The values are not two readings of the same property. One describes the comparative scale of the dipole source; the other describes mean field strength at the equator. The appropriate conclusion is not that one figure must be wrong, but that each needs its label and comparison basis.

Magnetosphere: a region shaped by more than the field

A magnetosphere is the space around a planet in which its magnetic environment has a major influence. Its boundary is affected by incoming solar wind as well as by the planet’s field and plasma, so a large magnetosphere does not automatically mean a proportionally stronger local field. Jupiter’s sunward magnetosphere reaches roughly 1–3 million kilometers, varying with conditions, and its magnetotail extends more than 1 billion kilometers, according to NASA. These are distances, not field-strength measurements. NASA’s Jupiter facts page.

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The sunward boundary and the tail describe different directions. The boundary facing the Sun responds to the incoming solar wind and can vary; the tail stretches away from the Sun. Jupiter’s quoted dimensions therefore convey the remarkable reach of its magnetic environment, but they should not be converted into a field-strength ratio. The same caution applies when comparing magnetospheres across planets: their extents depend on interactions and conditions, not only the value of a local field.

Why do Earth, Jupiter, and Saturn generate different magnetic fields?

Each planet’s internal magnetic field is associated with moving, electrically conducting material inside it, but the conducting material differs between Earth and the two gas giants. Rotation and the structure of those interiors also matter; a comparison of field strength alone cannot describe the dynamo that produces it.

A dynamo is the process by which motion in electrically conducting material sustains a magnetic field. The materials, depths, and planetary conditions are not interchangeable across Earth and the giants. The comparisons below describe the broad interior explanations; they do not mean that a spacecraft has directly visited or sampled the dynamo region.

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Earth’s liquid-core dynamo

Earth’s magnetic field is generated by a dynamo associated with moving, electrically conducting liquid in its core. The core is not directly sampled by a spacecraft, so illustrations of its magnetic dynamo are model-based descriptions of a deep interior process. Earth’s field is the reference unit for the dipole-moment figures in NASA Goddard’s comparison, and its equatorial-field entry is 0.31 gauss.

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Metallic hydrogen inside Jupiter and Saturn

NASA describes Jupiter’s rapidly rotating, electrically conducting liquid metallic hydrogen as the material acting as a dynamo. Saturn also has an internal liquid-metallic-hydrogen layer. In both giants, the relevant conducting region is deep inside the planet, not a surface feature or an external magnetic shell.

A NASA/JPL-Caltech/SwRI illustration based on Juno-related work gives modeled dynamo-core scales of 0.54 Earth radii for Earth and 0.81 Jupiter radii for Jupiter. Those are fractions of each planet’s own radius, not distances in kilometers, and they are model interpretations rather than locations a probe reached. The graphic places Jupiter’s modeled dynamo within convective metallic hydrogen. NASA’s Earth-and-Jupiter magnetic-fields graphic.

The radius units in that illustration are easy to misread: 0.54 Earth radii means a modeled scale expressed relative to Earth’s radius, while 0.81 Jupiter radii uses Jupiter’s radius. They are not directly comparable kilometer measurements unless converted, and the graphic is describing modeled interior scales rather than the reach of the external magnetosphere. Keeping those two kinds of “size” separate avoids confusing a planet’s internal dynamo region with the space its magnetic field influences.

How are the magnetic axes tilted?

Earth’s and Jupiter’s dipole axes are tilted by roughly 11° and 10° relative to their respective spin axes. Saturn’s dipole is almost aligned with its spin axis. That geometry is a separate property from how a planet’s spin axis is oriented relative to its orbit.

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The comparison table lists the specific approximate tilts from NASA Goddard’s historical comparison: 11.3° for Earth, 9.6° for Jupiter, and about 0° for Saturn. “Almost aligned” is more accurate than “perfectly aligned.” A NASA model lists Saturn’s dipole tilt as 0.0°, but also describes a nonzero dipole offset and higher-order magnetic components. A simple dipole-axis number therefore does not mean that Saturn’s entire magnetic field is perfectly centered or has no complexity. NASA Goddard’s comparison and Saturn field model.

It is also important not to mix up magnetic-axis tilt and spin-axis tilt. The table’s angles compare a planet’s magnetic dipole axis with its own rotation axis. A planet’s rotation axis relative to its orbit is a different angle and answers a different question. For this comparison, the useful takeaway is that Earth and Jupiter have appreciable dipole tilts, while Saturn’s large-scale dipole is exceptionally close to aligned with its spin axis.

Saturn’s near alignment does not mean that the whole magnetic field is a perfectly centered bar-magnet pattern. The model includes an offset and higher-order components, which add detail beyond the simple dipole tilt. “Almost aligned” describes the main axes; it does not erase those other features.

How do moons and rotation shape the giant planets’ magnetospheres?

At Jupiter and Saturn, a magnetic environment includes plasma supplied by moons as well as the planet’s internal field and the solar wind. The details differ by planet, and describing one system should not be taken to mean that the other has no plasma disk or is unaffected by solar wind.

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Jupiter: rapid rotation and material from Io

NASA’s 2022 Jupiter technical handbook identifies magnetic tilt, rapid rotation, and Io as three major influences on Jupiter’s magnetic environment. Io supplies material that forms a plasma torus around Jupiter. Rapid rotation helps spread that plasma into a disk, adding a changing, plasma-rich component to the magnetosphere. This helps explain why Jupiter’s magnetic environment is not simply a static dipole scaled up from Earth’s.

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These influences work together: Jupiter’s internal field provides the magnetic setting, the fast spin affects how plasma is distributed, and material from Io supplies an important part of that plasma. The torus and disk are not another measurement of the 4.28-gauss equatorial field. They describe material and structure within the magnetosphere, which is why a description of Jupiter’s system needs more than a single field-strength number.

Juno observations also connect electrons moving along the magnetic connection between Jupiter and Io with Jovian radio emissions. That connection is an example of how a moon can participate in the planet’s magnetic environment, rather than merely orbiting inside it. NASA’s Jupiter facts page also notes intense charged-particle radiation near the planet that can damage spacecraft. The radiation environment is a practical consequence for missions, but it is not another way of stating the field-strength figures in the table. NASA’s Jupiter facts page.

Saturn: rings, moons, and plasma

Saturn’s magnetosphere encompasses its rings and many of its moons. Cassini observed the magnetic environment interacting with material from the rings and moons, with Enceladus an important source. The system is comparatively aligned in its large-scale dipole geometry, but that does not mean it is empty of plasma or unaffected by changing external conditions.

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As at Jupiter, the magnetosphere is not just the planet’s internal field considered in isolation. The rings, moons, plasma, and incoming solar wind all belong in a careful description of the surrounding environment. The available comparisons do not justify saying that Saturn has no plasma disk, nor that solar wind never matters to the giant planets. They do support the more specific point that moon-supplied material helps shape Saturn’s environment and that Enceladus is an important source.

NASA’s Cassini science summary quotes Marcia Burton, a magnetospheres and plasma science investigation scientist at NASA’s Jet Propulsion Laboratory: “Measurements from Cassini have totally changed our understanding of Saturn’s magnetosphere, yet many questions still remain,” NASA’s Cassini magnetosphere overview.

What do the differences mean for aurorae and spacecraft?

All three planets have aurorae, but there is no single mechanism that explains every auroral event across all three. Charged particles and magnetic fields are central, while the source and motion of the particles differ by planet and can involve solar wind, rotation, or moon-supplied material.

NASA describes Earth’s auroral particles in connection with the solar wind. At least some Saturn aurorae, by contrast, appear substantially influenced by moon-derived particles and planetary rotation, rather than being controlled chiefly by the solar wind; the mechanism is not wholly settled. Jupiter’s connection to Io provides another example of moon-related magnetic activity. These qualifications matter: a statement about some aurorae at Saturn is not a universal explanation for all Saturn displays, and an explanation for one giant planet should not be applied automatically to another. NASA’s Saturn facts page.

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For spacecraft, Jupiter’s intense charged-particle radiation is an operational hazard reported by NASA, while the enormous dimensions of the magnetosphere define a far-reaching environment missions may encounter. Neither point means that the field is uniform throughout that space. The magnetosphere is structured by the planet’s field, rotation, plasma sources, and interactions with the solar wind.

For a reader comparing the three worlds, the practical distinction is this: field strength describes a specified magnetic measurement, while radiation and auroral activity are outcomes of particles moving and interacting within a more complex environment. Jupiter’s radiation warning is a spacecraft concern; it should not be used as a substitute for the table’s field values. Likewise, the presence of aurorae on all three planets does not imply that their particle sources or dynamics are identical.

Can a classroom magnet model show the difference?

A bar magnet and iron filings can help illustrate the shape of a magnetic field, but they cannot reproduce Jupiter’s actual field strength, its scale, or its plasma disk. NASA’s Magnetic Math classroom activity uses a bar magnet and iron filings to model a magnetosphere, making it a useful analogy when its limits are made clear. NASA’s Magnetic Math activity.

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In a simple demonstration, filings reveal a pattern around a magnet; they do not measure the field strength in gauss. A compass can indicate local field direction, but a small classroom magnet does not stand in for a planet’s conducting interior, rotating plasma, or interaction with the solar wind. The demonstration is best used to understand why magnetic fields have structure, not to infer a planet-to-planet strength ratio.

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For a home or classroom activity, a basic bar-magnet-and-iron-filings magnetic-field kit is an optional way to make the pattern visible. Use the filings as a visualization tool, not as a measuring instrument or a scale model of Jupiter. A compass is an optional accessory if the goal is to explore direction around Earth or a nearby magnet. A magnetic-field meter is a more specialized option only if its specifications are suitable for measuring Earth’s relatively weak field; there is no basis here for claiming that a particular meter can measure Jupiter or Saturn from Earth. No specific product, price, or tested instrument is needed to understand the comparison.

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Frequently asked questions

Is Jupiter’s magnetic field stronger than Earth’s?

Yes, in NASA Goddard’s historical comparison, Jupiter’s mean equatorial field is 4.28 gauss versus Earth’s 0.31 gauss, about 14 times as large on that specific metric. Its dipole moment is about 20,000 times Earth’s in the same table. Other NASA pages use broader comparisons, so state the metric when giving a ratio.

Why does one NASA page say Jupiter’s field is 16–54 times Earth’s?

NASA’s Jupiter facts page gives that broader comparison without defining it as the mean equatorial-field metric used in NASA Goddard’s table. It is therefore best quoted with the page and wording attached, rather than substituted for the table’s specific equatorial values.

Why does NASA say Saturn’s magnetic field is 578 times Earth’s?

NASA’s Saturn facts page gives the 578-times figure but does not specify there that the comparison uses mean equatorial field. The source does not establish that it is directly comparable to the 0.22-gauss Saturn entry in NASA Goddard’s table.

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Why does Saturn have a weaker listed equatorial field but a larger magnetic moment than Earth?

Mean equatorial field and dipole moment are different quantities. NASA Goddard’s table lists Saturn at 0.22 gauss for mean equatorial field, compared with Earth’s 0.31 gauss, while listing its dipole moment at about 600 Earth units. The figures can differ because they describe different aspects of the magnetic environment.

Is Saturn’s magnetic field tilted?

Its main dipole axis is almost aligned with its spin axis. NASA Goddard’s comparison gives about 0° of tilt, and a model lists 0.0°, but “perfectly aligned” would be too absolute: the model also includes a nonzero dipole offset and higher-order components.

What makes Jupiter’s magnetosphere so large?

NASA reports a sunward reach of roughly 1–3 million kilometers, varying with conditions, and a magnetotail extending more than 1 billion kilometers. Its magnetosphere is shaped by the planet’s field, plasma, rotation, Io’s material, and the solar wind. Those distances describe extent, not local field strength.

Does Jupiter’s magnetic field make radio waves?

Juno observations connect electrons traveling along the Jupiter–Io magnetic connection with Jovian radio emissions. This is a specific observed connection, not evidence that all Jovian radio emissions share one cause.

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Can iron filings show how strong Jupiter’s magnetic field is?

No. Filings can make a magnetic-field pattern visible around a nearby magnet, but they do not provide a calibrated measurement in gauss or recreate a planet’s scale and plasma environment.

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Frequently Asked Questions

Is Jupiter’s magnetic field stronger than Earth’s?

Yes, in NASA Goddard’s historical comparison, Jupiter’s mean equatorial field is about 14 times Earth’s, and its dipole moment is about 20,000 times Earth’s. Those are separate measures, so the metric should accompany any ratio.

Why does one NASA page say Jupiter’s field is 16–54 times Earth’s?

NASA’s Jupiter facts page gives that broader comparison without defining it as the mean equatorial-field metric used in NASA Goddard’s table. Quote it with its source and wording rather than substituting it for the table’s specific equatorial values.

Why does NASA say Saturn’s magnetic field is 578 times Earth’s?

NASA’s Saturn facts page gives the 578-times figure but does not specify there that it uses mean equatorial field. It is not established as directly comparable to the table’s 0.22-gauss Saturn entry.

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Why does Saturn have a weaker listed equatorial field but a larger magnetic moment than Earth?

Mean equatorial field and dipole moment measure different aspects of a magnetic environment. The table lists Saturn’s mean equatorial field as 0.22 gauss and its dipole moment as about 600 Earth units; those values are not contradictory.

Is Saturn’s magnetic field tilted?

Saturn’s main dipole axis is almost aligned with its spin axis. A model lists 0.0° of tilt, but also a nonzero dipole offset and higher-order components, so “perfectly aligned” is too absolute.

What makes Jupiter’s magnetosphere so large?

Its extent reflects the planet’s magnetic environment and interactions involving plasma, rapid rotation, Io, and the solar wind. NASA gives a variable sunward reach of roughly 1–3 million kilometers and a tail extending more than 1 billion kilometers; these are distances, not field-strength values.

Does Jupiter’s magnetic field make radio waves?

Juno observations connect electrons traveling along the Jupiter–Io magnetic connection with Jovian radio emissions. That is a specific observed connection, not a claim that all Jovian radio emissions share one cause.

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Can iron filings show how strong Jupiter’s magnetic field is?

No. Filings reveal a pattern around a nearby magnet but do not provide a calibrated field-strength measurement in gauss or recreate a planet’s scale and plasma environment.

The Bottom Line

Jupiter leads Earth and Saturn in both mean equatorial field and dipole moment in NASA Goddard’s comparison, but those are different measurements. Saturn is the reminder to keep the metric visible: its listed equatorial field is weaker than Earth’s even though its dipole moment is much larger. Earth and Jupiter have tilted dipole axes, Saturn’s is nearly aligned, and all three magnetic environments are shaped by more than their internal fields alone.

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