About Jupiter's Family Secrets
Secrets of the Solar System Family
Our solar system is a family of planets, dwarf planets, comets, and asteroids orbiting our Sun, each harboring clues of our common origins, with their disparate compositions and characteristics.
How do scientists discover those secrets? Ancient civilizations studied the skies and noted the strange travelings of "wanderers," or "planetes" in Greek, which seemed to move against the background of familiar constellations. Telescopes allowed astronomers to view the surfaces of planets; spacecraft instruments now allow us to infer information about the interiors of planets. Instruments like radar, orbital mapping devices, and others that detect wavelengths of light invisible to the human eye are some of the tools that allow spacecraft to explore other worlds.
NASA's Juno mission to Jupiter launched in 2011 and will not only investigate the deepest mysteries of Jupiter's unique personality, but will also plumb the secrets of our solar system's origins.
Our Solar System Was Born from a Cloud of Gas and Dust
Like all families, the members of our solar system family share a common origins story. Their story started even before our solar system formed 4.6 billion years ago.
The prelude to this first chapter was when our universe (all space and time and matter and energy) was born in the Big Bang about 13.7 billion years ago. The universe began as a single point, rapidly expanding into space and time; as the intense radiation that filled the space began to cool, elementary particles began to fill it. Eventually, particles combined and formed clouds of gas and eventually stars and galaxies. More information about the Big Bang is at http://www.cfa.harvard.edu/seuforum/bigbanglanding.htm
The first stars lived out their lives and eventually exploded, sending "star stuff" out into the cosmos. That original stellar material was recycled as another generation of stars, and many of these, too, exploded at the end of their lives. Our Sun is thought to be a third–generation star and our entire solar system is made of the recycled star stuff of previous star generations. Our Sun is a granddaughter of the very first stars!
Our solar system began forming within a concentration of interstellar dust and hydrogen gas which contracted into a solar nebula, forming the proto-Sun and planetesimals that eventually joined into planets. Check out how the planets formed and changed through a series of images at the "Evolution of our Solar System" timeline.
Scientists still have many questions about our solar system's story, and Juno will help scientists begin to piece together the missing clues: How did the planets form so quickly (at least in cosmic terms)? Did the planets form in their present locations, or did the giant planets form closer to the Sun and, through complex gravitational interactions, migrate to their orbits of today?
The Juno Mission Will Unlock Jupiter's Family Secrets
At more than twice the mass of all the other planets combined, Jupiter is the patriarch of our planet family. It grew large enough to capture and hold onto the materials of the solar nebula, so its mixture of about 90% hydrogen and 10% helium by percent volume (with some methane, water, and ammonia mixed in) reflects the composition of the primordial mixture that produced all the planets. Yet, its composition is not exactly like the primordial mixture, leaving scientists uncertain about how exactly Jupiter, and by extension, the solar system, formed. Better understanding Jupiter's traces of methane, water, and ammonia will help scientists piece together exactly how a collection of gas and dust came to form the planets we see today.
Juno will use sophisticated instruments to spy deep into Jupiter's atmosphere in wavelengths of light invisible to the human eye, and it will gather information about the trace components water and ammonia. By measuring how its orbit is very slightly altered by the gravity of the planet, Juno will infer just how massive Jupiter's core is, which will provide additional clues about how Jupiter captured heavy enough materials in its infancy to grow so large. The very stuff of Jupiter holds clues to understanding the story of our solar system's birth!
Jupiter's Atmosphere –Jupiter's clouds shroud a very turbulent place. The immense pressure of the planet's bulk crushed the interior as it formed (and possibly still does as Jupiter continues to contract) and the resulting heat is still leaking from the planet. Jupiter is far from the Sun, but this internal heat warms the planet and plays a major role in its weather. Jupiter radiates twice as much infrared energy as it receives from the Sun! Its core temperature may be about 43,000ºF (24,000°C) — hotter than the surface of the Sun. This heat leaks up through the liquid metallic hydrogen and liquid hydrogen layers to supply energy to the atmosphere. Like a pot of soup on a hot stove, atmospheric gases boil up from the warm bottom layers to the cooler upper layers; temperatures are–261°F(–163°C) at the top of the atmosphere. Juno will map the atmosphere's temperature at different depths.
While it orbits the Sun only once every 12 years, Jupiter spins on its axis once every 10 hours. The rapidly spinning planet generates five jet streams in each hemisphere that produce Jupiter's unique banded appearance. Earth has only about four dynamic jet streams, two — sometimes three — in each hemisphere, which all travel from west to east. Wind speeds are high, up to 330 miles (530 kilometers) per hour, and alternate direction from eastward to westward with latitude. Lightning, produced as ice particles within storms rub past each other, is frequent. The Great Red Spot is a massive storm system larger than the diameter of Earth that has been raging for at least several hundred years.
Both magnetic fields originate from processes deep in each planet's interior. Earth's is generated from the electric current caused by the flow of molten metallic material within its outer core. Jupiter's gases are crushed to such incredible pressures that they are forced beyond the common states of liquid, solid, or gas that we find on Earth. One such a layer inside Jupiter is metallic hydrogen, and the electric current caused by swirling movements in this substance produces a magnetic field so large that its tail end ("magnetotail") extends past the orbit of Saturn.
Juno will map Jupiter's magnetic field. Its unique polar orbit will carry it above the poles to study Jupiter's auroras and how the magnetic field slams invisible charged particles into the atmosphere to produce the beautiful lights. Juno will measure the charged particles and the electric currents they create along the magnetic field lines. Juno will also "listen" for the radio signals given off by these particles as they move through the magnetic field. Its special "eyes" — an ultraviolet spectrometer — will "see" the aurora in a wavelength of light invisible to our eyes. JunoCam will take pictures of the planet, which scientists and students will use to study the poles.
Jupiter's Moons – Jupiter has its own family of at least 63 moons. Ganymede, the largest of Jupiter's moons, is bigger than the planet Mercury. Scientists suspect that the tiny moons Adrastea, Metis, Amalthea, and Thebe have slowly shed particles to create Jupiter's thin, dark rings.
Cousin Earth's Own Story Continues to Unfold
In the inner solar system, a distinct set of sibling planets formed from the primordial nebula: the inner, terrestrial planets Mercury, Venus, Earth, and Mars. These relatively small, rocky, dense planets lack the thick shroud of gases surrounding each of the giant planets, because they are heated by their closeness to the Sun and the blast of solar wind from the early Sun stripped them of their ices and gases.
The process of accretion that formed the rocky planets — bits and pieces gradually clumping together into larger and larger bodies — also left its mark on the planets and their moons. We can see craters on their surfaces.
Earth's Interior and Magnetic Field – Early in their histories, the accumulated heat from accretion, the continuing decay of their radioactive isotopes, and the energy of countless impacts made the terrestrial planets hot enough to separate into distinct layers (differentiate): Dense materials, like iron and nickel, sank to form cores; medium-density, rocky silicate materials formed mantles; and lighter rocks rose to the surfaces and cooled to form crusts. Earth's outer core is molten. Flow of this hot metallic material produces an electric current that generates our magnetic field.
Earth's Atmosphere – Over time, these planets regenerated their lost atmospheres though volcanic outgassing, with the larger planets, Venus and Earth, holding onto thicker atmospheres. Mars also regenerated an atmosphere, but the smaller planet's interior cooled more quickly. It is no longer outgassing at a sufficient rate; in addition, it no longer has a magnetic field to prevent the solar wind from stripping its gases away. Under the protection of their planet's magnetic field, Venus and Earth each accumulated comparatively thick atmospheres. Earth's was further modified by photosynthesis. Distinct from their giant gaseous cousins, however, the inner planets are mainly made of rock.
We are still uncovering the secrets of our own rocky inner planet, but we use it as the standard of comparison for our exploration of all other planets. Earth spins on its axis once a day and orbits the Sun once a year. All other planets are hot or cold compared to Earth's temperate surface temperatures, which range from about –125° to 130°F(–87° to 54°C). Our atmosphere traps energy from sunlight, creating a greenhouse effect that warms the surface. It also moderates the climate and protects the surface from some damaging components of solar radiation. The rotation axis is tilted, giving Earth its seasons. Earth has water, rock, and tectonic cycles, which are important for renewing nutrients. Earth is the only known planet with life, but we continue to search for other areas in our solar system that might harbor primitive life. Unique among all its siblings, it has a single, comparatively large natural satellite — the Moon.
The other members of our solar system family have their own secrets and delightfully diverse personalities. The following sections provide a brief overview of the other giant planets, the inner planets, as well as the smaller asteroids, dwarf planets, and comets that orbit our Sun. In addition, a table summarizing important statistics can be found in Family Portrait ... in Numbers.
Further information: These presentations are made by NASA scientists and engineers, to provide background information for program providers, and not to be used directly in youth programs. These external resources are not necessarily 508 compliant.
- Juno Mission to Jupiter: Unlocking the Giant Planet Story (7MB PowerPoint)
NASA's Juno Mission
- Jupiter: King of the Planets (6MB PowerPoint)
- Unlocking the Giant Planet Story with NASA's Juno Mission
NASA's Juno Mission
- The Magnetism of Jupiter: Erupting Volcanoes and Dazzling Auroras (13MB)
Dr. Fran Bagenal, University of Colorado at Boulder
- Jupiter Versus the Earth: Composition & Structure (1 MB PowerPoint)
Dr. Randy Gladstone, Southwest Research Institute
- Juno: Changing Views of Solar System Formation (10 MB PowerPoint)
Dr. Paul G. Steffes, Georgia Institute of Technology
- Exploring Jupiter with Radio Waves
Dr. W. S. Kurth, The University of Iowa
- NASA's New Horizons Mission (10 MB PowerPoint)
Steve Vernon, The John Hopkins University, Applied Physics Lab
- Explorers "Guide to the Solar System"
This NASA presentation is available to download in PowerPoint format and use in programs. The site also offers a suggested script as well as supporting activities.
- Exploring the Giant Magnetosphere of Jupiter (387 MB QuickTime Movie)
Dr. Fran Bagenal, University of Colorado at Boulder