This drawing shows how forming planets drew gas to themselves.
Click on image for full size
Image from: The New Solar System

How a proto-planet sweeps up nearby material

As shown in this picture, while they were forming in the solar nebula, the nuclei of the planets-to-be (called protoplanets) drew material to themselves from the cloud of gas and dust around them. The bigger protoplanets were able to attract even more gaseous material unto themselves.

Big protoplanets such as Neptune were positioned far out in the original nebula where there was less gas, and so these protoplanets were not able to sweep up as much gas as other giant planets.


Shop Windows to the Universe Science Store!

Enjoy your love of minerals and fossils through jewelry! We have beautiful Nature's Own jewelry in our online store, including earrings, necklaces, and pendants!

Windows to the Universe Community

News

Opportunities

You might also be interested in:

Hematite with Rutile

Check out our online store - minerals, fossils, books, activities, jewelry, and household items!...more

How the Solar System may have formed from a spinning cloud

Scientists think that the solar system formed out of a spinning cloud of hydrogen and helium gas. Because the cloud was spinning, it flattened into a frisbee shape, just like a ball of pizza dough becomes...more

Neptune's Present Great Dark Spot

This image shows the new Great Dark Spot of Neptune, which was discovered using the Hubble Space Telescope. The image shown here, shows a "hole" in the clouds of Neptune in pink, in the northern hemisphere,...more

A Look at the History of Neptune's Atmosphere

The giant planets have definitely changed since their formation. But how much remains to be seen. Most of the original air of the giant planets remains in place. (The earth-like planets lost most of their...more

Neptune's Cirrus Clouds

This image shows some clouds known as "cirrus" clouds, extending for many kilometers across the face of Neptune. These clouds are very high up, for they can be seen to cast shadows on the lower clouds,...more

Neptune's Smog Hazes

This image of Neptune uses false colors to show where the smog is. The smog of Neptune can be seen in red along the edge of the image. These hazes of smog are found at very high altitudes, over the clouds...more

A Look at Neptune's Clouds

Like Jupiter and all the giant planets, Neptune's appearance shows a striped pattern of clouds. Other cloud shapes seen over time include a small dark spot, the "scooter" and the Great Dark Spot. The Great...more

Discover Neptune

If you had a quiz question in school that asked what year Neptune was discovered, you'd probably choose 1846. But Neptune wasn't discovered the way all the other planets in our solar system were. Astronomers...more

Shop Windows to the Universe

Coprolites are available in our online store, along with other minerals and fossils, books, activities, jewelry, and household items.

Generous sponsorship of Windows to the Universe is provided by the Hewlett Foundation, the American Geological Institute, the American Geophysical Union, the National Science Foundation, NASA, NCAR, and the CISM and CMMAP projects. NASA CMMAP AGU CISM NCAR Hewlett AGI NSF