Discoveries - Why a Space Telescope?
Planets being born in knots of dust. An unknown energy propelling the expansion of the universe. Shattered comets and misshapen asteroids. Galaxies that crash together to remake themselves. Faint, distant glimpses of light from the universe’s most distant collections of stars.
For more than 25 years, the Hubble Space Telescope has brought the wonder, beauty and mysteries of the universe to Earth, spinning pictures out of light that have transformed our understanding of the universe.
With over 1.5 million observations and counting, Hubble continues to trek above Earth’s surface, free of the light-distorting and blocking effects of our planet’s atmosphere, beaming home data that reveals the answers to some of our most critical questions about the cosmos.
Why a Space Telescope?
Hubble was designed as a general purpose observatory, meant to explore the universe in visible, ultraviolet and infrared wavelengths. To date, the telescope has studied more than 40,000 cosmic objects, providing views astronomers were unable to capture from the ground.
In addition to blocking certain wavelengths of light altogether, Earth’s atmosphere is made up of shifting pockets of air that cause the twinkling appearance of stars in the night sky. This motion blurs images captured by telescopes on the ground. Hubble was placed into orbit above the atmosphere to avoid these effects.
Though Hubble’s mirror is much smaller than those found in the largest ground-based observatories, the telescope’s unique position above Earth’s atmosphere gives it incredible clarity. As the telescope orbits Earth, its mirror gathers light from the cosmos, collecting images and data. For some of Hubble’s deepest images, the telescope has stared at the same point in the sky for days, trying to capture as much of the dim glow of the far universe as possible.
Cosmic Revelations
When Hubble was launched, the age of the universe was known to be somewhere between 10-20 billion years old. By examining a certain class of stars that can be used to define distance, Hubble was able to help narrow that broad figure down to approximately 13.8 billion years, a number now used to understand the timeline and development of stars, galaxies and more.
Hubble has uncovered supermassive black holes lurking in the hearts of galaxies and helped map the presence of elusive dark matter around galaxy clusters. But one of its strangest discoveries was the revelation that the expansion of the universe is speeding up, driven by the presence of a still-unidentified and previously unknown “dark energy.” With its ability to bring pristine images of the universe to Earth, Hubble has often shown humanity how much it has still to learn about the cosmos.
Hubble’s Time Machine
Space is so immense that it takes even light considerable time to travel the vast expanses between objects. The light from Earth’s Moon takes about 1.3 light-seconds to reach us, so when we look up at the Moon in the sky, we see it as it appeared 1.3 seconds ago.
The light of the most distant cosmic objects began traveling through space billions of years ago. When it finally arrives in our corner of the universe, it shows us the universe as it was in the distant past. By capturing the faint light of the early universe, Hubble can see galaxies as they were billions of years ago, showing us how galaxies developed and evolved over time.
We can’t watch galaxies or stars change ― they evolve on a time scale of millions and billions of years. But by viewing them at different stages of their existence, Hubble has helped demonstrate how galaxies change and grow through interactions and collisions. It’s given us snapshots of stars at different stages of stellar life, and shown them coalescing and igniting in clouds of gas and dust, breathing out outer layers as nebulas, and exploding as supernovae.
Planets Near and Far
Hubble has been used to probe everything from the weather on planets in our solar system to the birth of planets around other stars. It’s examined the composition of the atmospheres of these extrasolar planets, or “exoplanets,” and may have captured one of the first visible-light images of such a planet.
Hubble’s ringside seat to cosmic events has made it an essential witness to events in our own solar system, such as comet and asteroid impacts on Jupiter, storms and auroras on our neighboring planets, disintegrating asteroids, and passing comets. Our cosmic backyard still holds many surprises, and Hubble has found rings and moons around Uranus and moons around Pluto. Because of Hubble, we have a much better understanding of what our solar system truly looks like, and how it works.
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