What does the CARMA telescope do?

What does the CARMA telescope do?

CARMA will be capable of both high resolution and wide-field imaging, covering a range of angular scales unmatched by any current or planned millimeter-wave instrument. The high sensitivity, sub-arcsecond angular resolution and excellent uv-coverage of CARMA will ensure major advances in studies of the universe.

What type of telescope is CARMA?

The Combined Array for Research in Millimeter-wave Astronomy (CARMA) was an astronomical instrument comprising 23 radio telescopes, dedicated in 2006….Combined Array for Research in Millimeter-wave Astronomy.

Part of Owens Valley Radio Observatory
Altitude 2,196 m (7,205 ft)
Telescope style radio interferometer
Website www.mmarray.org

Where is the CARMA telescope?

Located on a high-altitude site in the Inyo Mountains of California, CARMA is currently the most powerful millimeter array in the world, with unmatched imaging capabilities.

What has the CARMA telescope discovered?

For example, CARMA revealed the evolution, in the spiral galaxy M51, of giant molecular clouds (GMCs) driven by large-scale galactic structure and dynamics. CARMA was used to show that giant molecular clouds grow through coalescence and then break up into smaller clouds that may again come together in the future.

Who made the Carma telescope?

The Combined Array for Research in Millimeter-Wave Astronomy (CARMA), a joint venture of the California Institute of Technology, the University of California at Berkeley, the University of Maryland and the University of Illinois, was created by moving the six 10-meter telescopes at Caltech’s Owens Valley Radio …

How does the VLA telescope work?

The VLA is an interferometer array, using the combined views of its 27 antennas to mimic the view of a telescope as big across as the farthest distance between its antennas. For the VLA, this can range from less than a mile to over 22 miles across!

Where is Hubble telescope now?

Launched on April 24, 1990, aboard the Space Shuttle Discovery, Hubble is currently located about 340 miles (547 km) above Earth’s surface, where it completes 15 orbits per day — approximately one every 95 minutes.

Can anyone look through the Hubble telescope?

Unlike on many previous NASA space science missions, anyone can apply for observing time on the Hubble Space Telescope.

What is the largest telescope array?

The world’s most powerful radio telescope, in its combination of sensitivity, resolution, and versatility, is the Very Large Array (VLA) located on the plains of San Agustin near Socorro, in central New Mexico, U.S. The VLA consists of 27 parabolic antennas, each measuring 25 metres (82 feet) in diameter.

Where is the largest telescope array?

The Atacama Large Millimeter/submillimeter Array (ALMA) is a $1.3 billion collaboration between North America, Europe and Asia, built high on a mountain in Chile’s Atacama desert.

What will happen to the Hubble telescope after 2040?

According to the European Space Agency’s HST website, www.spacetelescope.org, “As such, there is no set date for Hubble’s retirement. Hubble will continue to work for as long as its components operate and it provides a good service to the scientific community.”

What happened to the Carma telescope?

The telescopes ceased operation in April 2015 and were relocated to the Owens Valley Radio Observatory for storage. The Atacama Large Millimeter Array in Chile has succeeded CARMA as the most powerful millimeter wave interferometer in the world.

What is the height of the CARMA observatory?

Location. According to the CARMA observatory catalog, the median height of all telescope pads was at an elevation of 2196.223 m (7205.807 ft). The observatory was located in the Inyo Mountains to the east of the Owens Valley Radio Observatory, at a site called Cedar Flat, accessed through Westgard Pass.

How many telescopes are in the OVRO array?

Six telescopes each 10.4 meters (34 ft) in diameter. These were part of the Millimeter Array at the OVRO site operated by Caltech. They were moved to Cedar Flat in the Spring of 2005. Nine telescopes each 6.1 m (20 ft) in diameter.