Home Table of Contents About the Authors Glossary Buy This Book Joseph Henry Press







Motion | Pages 44-45 | (back to unlinked version)

After hundreds of millions of years, the two galaxies may merge External Link: Images and descriptions of scientific studies of one such ``blob,'' NGC 7252. into a disturbed and disrupted blob. This scenario may be in our future.


cubes by shaking it violently. Io is scarred by fresh eruptions of molten sulfur and other minerals, which completely repave the moon's surface every few dozen years.

The next moon outward, Europa External Link: List of Europa images and movies., also is heated by Jupiter's tides, but less vigorously. It may be warmed enough to maintain a deep ocean of liquid water beneath its icy cracked crust. This is tantalizing, for many biologists believe that life on Earth began in the oceans. If the right conditions exist, Europa External Link: List of Europa images and movies.'s dark seas could even now be nurturing extraterrestrial life--without the Sun as a source of energy.

Some of nature's most spectacular displays of cosmic mayhem arise from tidal interactions on a much larger scale. Entire galaxies can collide, drawn together by their mutual gravitational pulls. The gravity of each galaxy tugs much more strongly on stars in the nearer side of the other galaxy. These tidal forces stretch the original structures into sweeping arcs and rings of stars. After hundreds of millions of years, the two galaxies may merge External Link: Images and descriptions of scientific studies of one such ``blob,'' NGC 7252. into a disturbed and disrupted blob. This scenario may be in our future. Our Milky External Link: A scientific visualization of what might happen if the Milky Way and Andromeda collide! Way and its neighbor, the Andromeda galaxy, are moving toward each other and could meet in about 5 to 7 billion years. By that time it won't matter for Earth because our Sun will have run out of its nuclear fuel.

Individual stars almost never smash together when galaxies collide. They are simply too far apart and too small compared with the vast distances between them. If there were four snails running loose in the continental United States for a billion years, two of them would be more likely to bump into each other than would two stars during a galactic collision. However, the oversized clouds of gas External Link: A gallery of such clouds, created by various cosmic processes. and dust in galaxies certainly do interact. The gravitational turmoil stirred by this process sets off new bursts of star formation, lighting up galaxies like a holiday display. We often see the brilliant blue External Link: Images and descriptions of scientific studies of one such ``starburst galaxy'' with long tidal tails, NGC 4038/4039 (the ``Antennae'' galaxies.) flares of newborn stars along graceful "tidal tails" flung into space during galactic collisions.

On the largest scale of all, the combined gravitational pulls of every object in the universe act to slow down the expansion of space-time that Edwin Hubble External Link: A glowing eulogy of this great astronomer, written by one of his greatest pupils. discovered in 1929. For years astronomers debated whether the universe contained enough mass to slow its own expansion to a halt. If so, gravity Internal Link:   would pull everything together in the ultimate "big squeeze." But it now appears that won't happen. Our universe probably is destined to expand forever, providing more than enough time for all the stars to burn out.


Galactic Tides

For the effects of gravitational attraction at the cosmic scale, we have only to look at the fanciful shapes of celestial objects such as the aptly named Antennae (right) and Cartwheel (page 46). Galaxies rarely exist in splendid isolation but instead travel through the universe interacting to varying degrees with other star systems. These interactions range from stressful near misses to head-on collisions, often with spectacular results.

Shown below are computer simulations that suggest how some so-called peculiar galaxies came to be. By calculating the gravitational interactions among each galaxy's stars, dust, and gas, scientists can reproduce such effects as the bridges of stars between galaxies and the streaming stellar tails that give the Antennae their name.

Creating Tidal Tails

This model of two disk galaxies colliding traces the gravitational effects on stars (yellow/white) and interstellar gas (blue) over about 1 billion years. The collision distorts the galaxies into an amorphous smudge (2). As the galaxies move apart, tidal tails curve away (3). Turning around on their orbit, the galaxies fall back toward each other (4), until they recollide (5) and merge into a single object that resembles the pair of galaxies known as the Antennae (above).



A Galactic Bull's-Eye

In this model, spanning about 350 million years, a small galaxy shoots through a larger disk galaxy along the disk's rotational axis (1, 2). Like the ripples caused by a rock tossed into a lake, a wave of energy expands outward, pushing gas and dust ahead of it into a ring (4), leaving a burst of star formation in its wake. As clumps of gas fall back toward the disk's center, they create radial spokes and an inner ring (5, 6), much like those seen in the Cartwheel (page 46).