Title: Three Radio Astronomy Futures:
1 - Three Radio Astronomy Futures
- ALMA, EVLA, SKA
Mark T. Adams Assistant Director, EPO National
Radio Astronomy Observatory http//www.nrao.edu
Osher Lifelong Learning Institute University of
Virginia 18 September 2008
2Electromagnetic Spectrum
The Domain of Radio Astronomy Wavelength 15
meters to 0.3 millimeter Frequency 20 MHz
to 1.0 THz 1 THz 1,000 GHz 1,000,000 MHz
3Green Bank Telescope
- Dedicated in 2000 in Green Bank, WV
- Located in National Radio Quiet Zone
- 100 x 110m dish 2 acres of collecting area
- Weighs 17M lbs largest moving structure on land
- Studies pulsars, complex molecules, neutral
hydrogen
4Very Large Array
- Built in 197s, Dedicated in1980
- 27 antennas in a reconfigurable array
Studies Black holes, proto-planetary disks around
young stars, Galactic Center, cosmology
5Very Long Baseline Array
- Operated from Socorro, NM
- Ten antennas
- Hawaii to the Caribbean
- Highest resolution astronomical telescope
- Dedicated 1993
6NRAO Technology Center
- Radio Astronomy technology signal processing
push state-of-the-art - NTC scientists, engineers, Technicians perform
the required Research Development
7The Invisible UniverseWhy Do Radio Astronomy?
- Radio complements other wavelengths
H o r s e h e a d N e b u l a
Optical Infrared Radio
8The Invisible UniverseHydrogen
Optical image of M81 Group (DSS)
9The Invisible UniverseCenter of our Galaxy
10Expanded Very Large Array
http//www.aoc.nrao.edu/evla
11Expanded Very Large Array
- Leverages the VLA to Enable the Next-Generation
cm-wavelength Telescope - builds on existing infrastructure 27 antennas,
Track, facilities, people - An International Collaboration United States,
Canada, and Mexico - Implements state-of-the-art technology
- Correlator
- wideband receivers 1 - 50 GHz
- fiber-optic data transmission system
- digital electronics
- Software
12EVLA Science Themes
Magnetic Universe
Measure the strength and structure of the cosmic
magnetic field
Obscured Universe
Sgr A
Image young stars massive black holes in dust
enshrouded environments
13EVLA Correlator
- WIDAR Wideband Interferometric Digital
Architecture - WIDAR is an Innovative method for digital
correlation of very wideband signals from a radio
interferometer - 40 x 1015 Ops / sec
invented by Brent Carlson Peter Dewdney at
Dominion Radio Astrophysical Observatory
14Atacama Large Millimeter/submillimeter Array
http//www.alma.nrao.edu http//www.alma.cl
15ALMA Science Schedule
- Key Science
- Cosmic Origins Planets, Stars, Galaxies
- The Cold Universe
- Timeline
- 1995 site testing in Chile Begins
- 1998 Design Development Start
- 2007 First ALMA Antennas Arrive in Chile
- 2010 First Science
- 2013 ALMA Fully Operational
16ALMA Location
- mm / sub-mm radiation is blocked by water in the
atmosphere - MM / sub-mm telescopes must be located at very
dry, high altitude sites - Chajnantor plain in northern chile (Atacama
Desert ) is the best
17Altiplano de ChajnantorRegion II, Chile
18ALMA Antennas in Chile
3 Melco Antennas
VertexRSI
19ALMA Transporter
Concept
Reality Sep 07
20Square Kilometre Array
- 1994 Community begins to Consider A Next-Gen
Radio Telescope With A Square Kilometre (250
Acres) of Collecting Area - Scientific Objectives
- Technology
- Cost
21Square Kilometre Array
- Key Science Projects
- Cradle of Life
- Gravity Tests Using Pulsars Black Holes
- Origin Evolution of Cosmic Magnetism
- Galaxy Evolution Cosmology
- Probing the Dark Ages
22Square Kilometre Arraynew technology
23Square Kilometre Array
- Pathfinder Technology development projects
underway in United States, Europe, South Africa,
Australia - Likely To Be 3 Separate SKA Telescope Systems
- SKA-Hi, SKA-Mid, SKA-Low
- Construction Cost 1- 2B USD for Each
- EVLA COMPLETE in 2012 SKA PATHFINDER
- SKA Fully Realized Operational 2025
- http//www.skatelescope.org
24Radio Astronomy discoveries Cosmic Microwave
Background Quasars Pulsars Gravitational
Lenses Dark Matter Masers Gravitational
Waves First Extra-solar PlanetsStay Tuned for
the EVLA, ALMA, SKA the Scientific frontiers
they will open