Showing posts with label Telescope. Show all posts
Showing posts with label Telescope. Show all posts

Saturday, 20 February 2016

NASA's Wide Field Infrared Survey Telescope (WFIRST)-With a view 100 times bigger than that of Hubble Space Telescope



NASA's Wide Field Infrared Survey Telescope
NASA's Wide Field Infrared Survey Telescope (WFIRST), illustrated here, will carry a Wide Field Instrument to capture Hubble-quality images covering large swaths of sky, enabling cosmic evolution studies. Its Coronagraph Instrument will directly image exoplanets and study their atmospheres.
Credits: NASA/GSFC/Conceptual Image Lab
After years of preparatory studies, NASA is formally starting an astrophysics mission designed to help unlock the secrets of the universe -- the Wide Field Infrared Survey Telescope (WFIRST).
With a view 100 times bigger than that of NASA’s Hubble Space Telescope, WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life.
NASA's Agency Program Management Council, which evaluates the agency's programs and projects on content, risk management, and performance, made the decision to move forward with the mission on Wednesday.


“WFIRST has the potential to open our eyes to the wonders of the universe, much the same way Hubble has,” said John Grunsfeld, astronaut and associate administrator of NASA’s Science Mission Directorate at Headquarters in Washington. "This mission uniquely combines the ability to discover and characterize planets beyond our own solar system with the sensitivity and optics to look wide and deep into the universe in a quest to unravel the mysteries of dark energy and dark matter.”
WFIRST is the agency's next major astrophysics observatory, following the launch of the James Webb Space Telescope in 2018. The observatory will survey large regions of the sky in near-infrared light to answer fundamental questions about the structure and evolution of the universe, and expand our knowledge of planets beyond our solar system – known as exoplanets.
It will carry a Wide Field Instrument for surveys, and a Coronagraph Instrument designed to block the glare of individual stars and reveal the faint light of planets orbiting around them. By blocking the light of the host star, the Coronagraph Instrument will enable detailed measurements of the chemical makeup of planetary atmospheres. Comparing these data across many worlds will allow scientists to better understand the origin and physics of these atmospheres, and search for chemical signs of environments suitable for life.
"WFIRST is designed to address science areas identified as top priorities by the astronomical community," said Paul Hertz, director of NASA's Astrophysics Division in Washington. “The Wide-Field Instrument will give the telescope the ability to capture a single image with the depth and quality of Hubble, but covering 100 times the area. The coronagraph will provide revolutionary science, capturing the faint, but direct images of distant gaseous worlds and super-Earths."


For more information about NASA's WFIRST mission, visit:

Saturday, 28 November 2015

The GIANT MAGELLAN Telescope -- Resolving power 10 times greater than the Hubble Space Telescope

            The Giant Magellan Telescope will be one member of the next class of super giant earth-based telescopes that promises to revolutionize our view and understanding of the universe. It will be constructed in the Las Campanas Observatory in Chile. Commissioning of the telescope is scheduled to begin in 2021.
           The GMT has a unique design that offers several advantages. It is a segmented mirror telescope that employs seven of today’s largest stiff monolith mirrors as segments. Six off-axis 8.4 meter or 27-foot segments surround a central on-axis segment, forming a single optical surface 24.5 meters, or 80 feet, in diameter with a total collecting area of 368 square meters. The GMT will have a resolving power 10 times greater than the Hubble Space Telescope. The GMT project is the work of a distinguished international consortium of leading universities and science institutions.



Quick info:

  • Completion target – 2021
  • Location – Las Campanas Observatory, Chile
  • Altitude of site – 8,254 feet (2,516 meters)
  • Height of telescope housing – 200 feet (61 meters)
  • Moving weight of telescope – 2,425,085 pounds (1,100 tons)
  • Weight of each finished mirror segment – 25,000 pounds (12.5 tons)
  • Diameter of each mirror – 28 feet (8.4 meters)
  • Effective diameter of all mirrors – 83.5 feet (24.5 meters)
  • Total collecting area of mirrors – 3,961 sq. feet (368 sq. meters)
  • Mounting type – altitude/azimuth
  • Wavelength sensitivity of telescope – Near infrared and visible (320–25000 nanometers)


For photo courtesy and more info visit following link