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  1. hubblesite.org › mission-and-telescope › the-telescopeThe Telescope | HubbleSite

    The telescope has beamed hundreds of thousands of celestial images back to Earth during its time in space. Hubble is a Cassegrain reflector telescope. Light from celestial objects travels down a tube, is collected by a bowl-like, inwardly curved primary mirror and reflected toward a smaller, dome-shaped, outwardly curved secondary mirror.

  2. Jan 15, 2019 · 3. For calculating we take t = d V t = d V, where V = Hd V = H d . But velocity isn't uniform for an object as distance also increases with time. And if velocity isn't constant the equation t = H d t = H d also isn't applicable. So how is the Hubble time the age of the universe intuitively? You're right, V V is not necessarily constant, and ...

  3. Dec 3, 2019 · The Hubble constant is a unit that describes how fast the universe is expanding at different distances from a particular point in space. It is one of the keystones in our understanding of the ...

  4. The age of the universe estimated in this way turns out to be just the reciprocal of the Hubble constant (that is, 1/H). This age estimate is sometimes called the Hubble time . For a Hubble constant of 20 kilometers/second per million light-years, the Hubble time is about 15 billion years.

  5. Mar 6, 2024 · NASA's Space Telescope Live provides an interactive way to explore the most accurate, up-to-date, publicly available information on current, past, and upcoming observations by NASA’s Hubble and Webb space telescopes. Identify, locate, and zoom into a map showing the latest target. Slew over to the next target and back to the previous one.

  6. By precisely determining the expansion rate, called the Hubble constant, the cosmic clock can be rewound and the age of the universe calculated. However, Edwin Hubble's estimates of the expansion implied that the universe was younger than the age of the Earth and the Sun. Hubble, therefore, concluded that the redshift phenomenon was an unknown ...

  7. The dynamical time scale, also called the crossing time, is the period of a galaxy orbit through the center of the cluster potential. The characteristic time scales are of order 10 9 years, much shorter than the Hubble time (the expansion time scale for the universe, taken as the inverse of the Hubble constant).

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