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The Hubble Space Telescope is one of the most important scientific instruments ever placed in orbit. Since its launch in 1990, it has taken sharp images above most of Earth's atmosphere, giving astronomers a clearer view of planets, stars, galaxies, and deep space. Its discoveries matter because they changed how scientists measure the size, age, and history of the universe. Hubble also turned distant cosmic objects into data that students and scientists can analyze with physics, math, and imaging techniques.

Hubble detects visible light, ultraviolet light, and near-infrared light with sensitive cameras and spectrographs. By measuring brightness, color, spectra, and positions over time, it helps determine distances, chemical compositions, motions, and ages of astronomical objects. Key discoveries include evidence for dark energy, improved measurements of the universe's expansion rate, detailed views of star birth and death, and deep-field images showing thousands of ancient galaxies. Its long lifetime makes it especially powerful because repeated observations reveal changes that a single image cannot show.

Key Facts

  • Hubble launched in 1990 and orbits Earth above most atmospheric blurring.
  • Hubble's mirror diameter is 2.4 m, which helps it collect faint light and resolve fine details.
  • Speed of light: c = 3.00 x 10^8 m/s.
  • Light travel time can be found with t = d/c.
  • Hubble's observations helped refine the Hubble constant, often written as v = H0d.
  • Deep-field images show that looking farther into space also means looking farther back in time.

Vocabulary

Hubble Space Telescope
A space-based observatory that studies the universe in visible, ultraviolet, and near-infrared light from orbit around Earth.
Spectrograph
An instrument that separates light into its wavelengths so scientists can identify motion, temperature, and chemical composition.
Redshift
The stretching of light to longer wavelengths, often caused by objects moving away or by the expansion of space.
Deep Field
A long-exposure image of a small patch of sky that reveals extremely faint and distant galaxies.
Dark Energy
A name for the unknown cause of the observed accelerated expansion of the universe.

Common Mistakes to Avoid

  • Thinking Hubble travels to distant galaxies, but it stays in orbit around Earth and observes light that reaches it from space.
  • Assuming Hubble sees only visible light, but it also detects ultraviolet and near-infrared light, which reveal objects and processes not obvious to human eyes.
  • Confusing image beauty with scientific evidence, because Hubble images are processed for clarity while the measurements come from calibrated brightness, spectra, and positions.
  • Treating lookback time as the current distance to an object, but an object's light travel time and its present distance can differ because the universe expands while the light travels.

Practice Questions

  1. 1 Hubble orbits about 540 km above Earth's surface. If Earth has a radius of 6370 km, what is Hubble's approximate distance from Earth's center?
  2. 2 A galaxy's light has traveled for 2.5 billion years before reaching Hubble. Using 1 light-year = 9.46 x 10^15 m, calculate the approximate distance the light traveled in meters.
  3. 3 Explain why placing a telescope above most of Earth's atmosphere improves astronomical observations compared with observing from the ground.