Skip to main content

ACT Telescope

Act telescope

Atacama Cosmology Telescope

The Atacama Cosmology Telescope

The goals of the ACT project are to study how the universe began, what it is made of, and how it evolved to its current state. This pursuit is part of the field of scientific cosmology in one which asks questions about the Universe on the largest and grandest scales. Over the past two decades, there has been a tremendous flourishing of the field, driven by many excellent astronomical measurements. This has led to the development of a precise and elegant understanding of cosmology.
The Atacama Cosmology Telescope (ACT) is a six-metre telescope on Cerro Toco in theAtacama Desert in the north of Chile, near theLlano de Chajnantor Observatory. It is designed to make high-resolution, microwave-wavelength surveys of the sky in order to study the cosmic microwave background radiation (CMB). At an altitude of 5190 metres (17,030 feet), it is one of the highest permanent, ground-based telescopes in the world.
ACT experiment has two main goals to further our knowledge of cosmology:
  1. To improve on the measurements of parameters which describe the very early universe
  2. To measure distant, large clusters of galaxies and their environments.



Erected in the (austral) autumn of 2007, ACT saw first light on 22 October 2007 with its science receiver, the Millimeter BolometerArray Camera (MBAC), and completed its first season in December 2007. It began its second season of observations in June 2008.





Comments

Popular posts from this blog

Planet - Mercury

Mercury is a planet in our solar system. It is the smallest of the eight planets. It is also the closest to the sun. Mercury goes around the sun the fastest of all the planets. Mercury has no moons. Mercury's physical characteristics Because the planet is so close to the sun,Mercury surface temperature can reach a scorching 840 degrees Fahrenheit (450 degrees Celsius). However, since this world doesn't have a real atmosphere to entrap any heat, at night temperatures can plummet to minus 275 F (minus 170 C), a temperature swing of more than 1,100 degrees F (600 degree C), the greatest in the solar system.  Mercury's elliptical orbit takes the small planet as close as 29 million miles (47 million kilometers) and as far as 43 million miles (70 million kilometers) from the sun. If one could stand on the scorching surface of Mercury when it is at its closest point to the sun, the sun would appear almost three times as large as it does when viewed from Earth ...

Black hole

A  black hole  is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a  black hole . Objects whose  gravitational fields  are too strong for light to escape were first considered in the 18th century by  John Michell  and  Pierre-Simon Laplace .  The first modern solution of general relativity that would characterize a black hole was found by  Karl Schwarzschild  in 1916, although its interpretation as a region of space from which nothing can escape was first published by  David Finkelstein  in 1958. Black holes were long considered a mathematical curiosity; it was during the 1960s that theoretical work showed they were a generic prediction of general relativity. The discovery of  neutron st...