Hubble Space Telescope and Its Successor

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    SWETA DAS

    0811012052

    ECE-A

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    How does a telescope work?

    Hubble History

    Deeper into Hubble

    Optical Assembly

    Scientific Instruments

    Spacecraft Systems

    Hubble Successor-JamesWebb SpaceTelescope How doesWebb contrasts Hubble?

    References

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    A telescope is an instrument that aids in observing distant objects by collecting

    electromagnetic radiation from them.

    Basic telescope

    Electromagnetic spectrum and earths transmittance

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    The Hubble Space Telescope (HST) is a space telescope that was carriedinto orbit by a Space Shuttle in 1990 and remains in operation. A 2.4 meter (about8 ft.) aperture telescope in low Earth orbit, Hubble's four main instruments

    observe in the near ultraviolet, visible, and near infrared. The telescope is named

    after the astronomer Edwin Hubble.

    Hubble's orbit outside the distortion of Earth's atmosphere allows it to takeextremely sharp images with almost no background light.

    Hubble's Ultra Deep Field image, for instance, is the most detailed visible

    light image ever made of the universe's most distant objects.

    Many Hubble observations have led to breakthroughs in astrophysics, such asaccurately determining the rate of expansion of the universe .

    Hubble is the only telescope designed to be serviced in space by astronauts.Between 1993 and 2002, five missions repaired, upgraded, and replaced systems

    on the telescope .It is expected to work until atleast 2014.

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    Hubble telescope mainly consists of 3 important parts to carry out itsmultiple missions

    Optical assembly

    Scientific instruments

    Spacecraft systems

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    Light enters Hubble's aperture and travels down

    the main baffle. A baffle is a surface which

    eliminates stray light.

    Light is reflected by the primary mirror which measures

    about 8 feet (2.4 meters) in diameter. Because of the

    concave shape, the primary mirror converges the light

    to the secondary mirror through a secondary baffle.

    The secondary mirror, measuring about 1 foot (0.3 m)

    in diameter receives the light. It in turn reflects

    the still-converging light back toward the primary

    mirror through a central baffle.

    The light travels through a hole in the primary mirror,

    to reach the focal plane, where the science instruments

    examine the light.

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    Hubble's scientific instruments work either togetheror individually to bring us stunning images from the

    farthest reaches of space. Presently, Hubble can

    accommodate five scientific instruments and

    three fine guidance sensors.

    Depending on the position of the instruments , they are classified as axial bays andradial bays.

    Axial bay houses 5 main instruments namely :

    Advanced camera for surveys(ACS)Corrective Optics Space Telescope Axial Replacement(COSTAR)

    Cosmic Origins Spectrograph(COS)

    Near Infrared Camera and Multi-Object Spectrometer(NICMOS)

    Space Telescope Imaging Spectrograph(STIS)

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    Radial bays houses

    Wide Field Camera 3(WFC3)3 Fine Guiding Sensors(FGS)

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    Several spacecraft support systems are required to keep Hubble functioningsmoothly in space.These systems are located around the body of the spacecraft

    and encompassed by the outer hull.

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    The James Webb Space Telescope is an infrared-detecting

    observatory that will soar through space at the Second Sun-Earth

    Lagrange Point, an orbit far beyond Earth's Moon.

    Webb's giant sunshield will protect it from stray heat and light,

    while its large mirror enables it to effectively capture infrared light,

    bringing us the clearest picture ever of objects that emit this invisible

    radiation early galaxies, just-forming stars, clouds of gas and dust,

    and much more.

    At this distant orbit, the Webb telescope is too far from Earth to

    have the protection of our planet's magnetic field, which blocks

    high-energy cosmic rays

    Webb has an ambitious design that tackles the two main challenges for an infrared telescope: it

    has to have a large mirror, in order to best capture the long infrared wavelength; and it has to be

    kept cold, in order to keep

    unwanted sources of infrared from interfering with the emissions it attempts to detect.

    Webb's most innovative component is its primary mirror, which will be folded up to fit inside

    the rocket that launches it into space, and unfold once it nears its orbit.

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    SIZE

    ORBIT

    Hubble is 13.2 m long and its max

    diameter is 4.2mWebbs sunsheild is 22m by 12m

    Hubble orbits the earth.Webb will sit at earth-sun L2 point

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    WAVELENGTH

    HOW FAR TO SEE?

    Webb works in infrared and some parts of visible region(0.6-.28micrometers) whereas Hubble

    works in ultraviolet and visible region (0.1-0.8microns)

    Hubble can see the equivalent of "toddler

    galaxies" and WebbTelescope will be able

    to see "baby galaxies".

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    The HST is arguably the most significant device ever devised and fielded.

    It has given us spectacular images of distant stars and galaxies.

    It accurately determined the age of the universe to be 13 to 14 billion

    years old.

    It showed that the universe is not only expanding but also accelerating.

    Eventually when Hubbles time will end it will be replaced by the Webb

    space telescope which is much better and bigger than its space

    counterpart.

    The discoveries that webb will make will give us an idea about the origin

    of many ancient and farthest stars and galaxies.It will help us in knowingour universe in a better manner.

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    http://hubble.nasa.gov/ncs-story/event-01.php

    http://www.nasa.gov/mission_pages/hubble/main/index.html

    http://en.wikipedia.org/wiki/Hubble_Space_Telescope

    http://hubblesite.org/

    http://en.wikipedia.org/wiki/James_Webb_Space_Telescope

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    THANK YOU