ARECIBO, Puerto Rico — A huge, already damaged radio telescope in Puerto Rico that has played a key role in astronomical discoveries for more than half a century completely collapsed on Tuesday.
The telescope's 900-ton receiver platform and the Gregorian dome — a structure as tall as a four-story building that houses secondary reflectors — fell onto the northern portion of the vast reflector dish more than 400 feet below.
The U.S. National Science Foundation had earlier announced that the Arecibo Observatory would be closed. An auxiliary cable snapped in August, causing a 100-foot gash on the 1,000-foot-wide dish and damaged the receiver platform that hung above it. Then a main cable broke in early November.
The collapse at 7:56 a.m. on Tuesday wasn't a surprise because many of the wires in the thick cables holding the structure snapped over the weekend, Ángel Vázquez, the telescope's director of operations, told The Associated Press.
"It was a snowball effect," he said. "There was no way to stop it.... It was too much for the old girl to take."
Ángel Vázquez explains the collapse of the Arecibo Observatory @SaveTheAO. 1/2 pic.twitter.com/7VCZNCFsA4
— Wilbert Andrés Ruperto (@ruperto1023) December 1, 2020
The collapse stunned many scientists who had relied on what was until recently the largest radio telescope in the world.
"It sounded like a rumble. I knew exactly what it was," said Jonathan Friedman, who worked for 26 years as a senior research associate at the observatory and still lives near it. "I was screaming. Personally, I was out of control. ... I don't have words to express it. It's a very deep, terrible feeling."
Friedman ran up a small hill near his home and confirmed his suspicions: A cloud of dust hung in the air where the structure once stood, demolishing hopes held by some scientists that the telescope could somehow be repaired.
Vázquez, the telescope operations director, said that it was extremely difficult to say whether anything could have been done to prevent the damage that occurred after the first cable snapped in August.
"The maintenance was kept up as best as we could," he said. "(The National Science Foundation) did the best that they could with what they have."
Installing a new telescope would cost up to $350 million, money the NSF doesn't have, he said, adding it would have to come from U.S. Congress.
Scientists worldwide had been petitioning U.S. officials and others to reverse the NSF's decision to close the observatory. The NSF said at the time that it intended to eventually reopen the visitor center and restore operations at the observatory's remaining assets, including its two LIDAR facilities used for upper atmospheric and ionospheric research, including analyzing cloud cover and precipitation data. The LIDAR facilities are still operational, along with a 12-meter telescope and a photometer used to study photons in the atmosphere, Vázquez said.
The telescope was built in the 1960s with money from the Defense Department amid a push to develop anti-ballistic missile defenses. It had endured hurricanes, tropical humidity and a recent string of earthquakes in its 57 years of operation.
The Hubble telescope: 30 years of photos from space
NASA's Hubble Space Telescope sent back its first image from space on May 20, 1990. Here are some of the iconic images Hubble has sent back since.
Crab Nebula

This image gives the most detailed view so far of the entire Crab Nebula ever made. The image is the largest image ever taken with Hubble's WFPC2 workhorse camera.
Seyfert's Sextet

This image from the Hubble Space Telescope shows a group of galaxies called the Seyfert's Sextet on June 26, 2000. Although the name of this grouping suggests that there are six, there are in reality only four galaxies in the group that are slowly merging into one.
Lagoon Nebula

This NASA Hubble Space Telescope image shows a pair of one-half-light-year-long interstellar "twisters," eerie funnels and twisted-rope structures, in the heart of the Lagoon Nebula, which lies 5,000 light-years away in the direction of the constellation Sagittarius. The central hot star, O Herschel 36 (lower right), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass.
Spiral galaxy NGC 4631

An image of NASA's Chandra X-ray Observatory and Hubble Space Telescope shows a halo of hot gas surrounding spiral galaxy NGC 4631 that is similar to the Milky Way galaxy, June 19, 2001. The orange color in the middle of the image represents ultraviolet radiation as observed by UIT, tracing massive stars in the galaxy.
Little Ghost Nebula

The Hubble Space Telescope took this image of a dying star named "NGC 6369" on Nov. 7, 2002. The star, also known as the "Little Ghost Nebula," is 2000 to 5000 light years from Earth and is similar in mass to our sun. The ghostly halo surrounding the star is caused by the shedding of the star's outer layers during the final stages of its life cycle.
Cone Nebula

The Cone Nebula, an innocuous pillar of gas and dust, is seen in this picture unveiled by astronomers on April 30, 2002.
Nebula IC 1396

Resembling a flaming creature on the run, this image exposes the hidden interior of a dark and dusty cloud in the emission Nebula IC 1396. Young stars previously obscured by dust can be seen here for the first time.
Cas A supernova

An image of a Cas A supernova reveals the remnants of a section of the upper rim of the youngest known supernova identified in our Milky Way galaxy. Dozens of tiny clumps near the top of the image are actually small fragments of the star, and each clump is approximately 10 times larger than the diameter of our solar system. The varying colors of the supernova are caused by glowing atoms.
Kepler's supernova

This image released Oct. 7, 2004, by NASA shows Kepler's supernova remnant produced by combining data from NASA's Hubble Space Telescope, Spitzer Space Telescope and Chandra X-ray Observatory. Kepler's supernova was first seen 400 years ago by sky watchers, including famous astronomer Johannes Kepler. The combined image unveils a bubble-shaped shroud of gas and dust that is 14 light-years wide and is expanding at 4 million miles per hour (2,000 kilometers per second).
Whirlpool Galaxy and Eagle Nebula

In this composite handout image released from the Hubble Space Telescope, the Whirlpool Galaxy and Eagle Nebula are seen April 25, 2005.
Pluto and its moons

This undated image taken by the Hubble telescope shows Pluto and its moons Charon, Nix and Hydra. The International Astronomical Union announced on Aug. 24, 2006, that it no longer considered Pluto a planet, a status it had held since its discovery in 1930.
Jupiter

A curtain of glowing gas is wrapped around Jupiter's north pole like a lasso Dec. 19, 2000, in a Hubble telescope photo. The curtain of light, called an aurora, is produced when high-energy electrons race along the planet's magnetic field and into the upper atmosphere. The electrons excite atmospheric gases, causing them to glow. The aurora resembles the same phenomenon that crowns Earth's polar regions.
Radiant Star

The Radiant Star, Sept. 13, 1996.
'Eskimo' Nebula

Hubble takes a look at the "Eskimo" Nebula in this March 6, 2000, image. This stellar relic, first spied by William Herschel in 1787, was nicknamed the "Eskimo" Nebula because, when viewed through ground-based telescopes, it resembles a face surrounded by a fur parka.
NGC 1999

Just weeks after NASA astronauts repaired the Hubble Space Telescope in December 1999, the Hubble Heritage Project snapped this picture of NGC 1999, a nebula in the constellation Orion. The Heritage astronomers, in collaboration with scientists in Texas and Ireland, used Hubble's Wide Field Planetary Camera 2 (WFPC2) to obtain the color image.
Saturn

These Hubble Space Telescope images, captured from 1996 to 2000, show Saturn's rings open up from just past edge-on to nearly fully open as it moves from autumn toward winter in its Northern Hemisphere, part of the course of its 29-year journey around the sun.
Mars

A comparison image of the planet Mars reveals that a global dust storm has engulfed the planet. The storm is comprised of fine dust and obscures all surface features.
Stingray Nebula

The Stingray Nebula as photographed by the Hubble Space Telescope April 2, 1998.
Supernova self-destruction

The self-destruction of supernova 1987-A(C) is shown in this composite image taken in September 1994, February 1996 and July 1997.
Hubble Space Telescope

This April 6, 1994, image taken by the Hubble Space Telescope shows stars that lie near the center of our galaxy some 25,000 light-years distant. But one object, the blue curved streak (upper right), is something much closer. An uncatalogued, mile-wide bit of rocky debris orbiting the sun only light-minutes away strayed into the cameras field while the image was being exposed.
Moons of Jupiter

This is a Hubble Space Telescope "family portrait" of the four largest moons of Jupiter.
Elliptical galaxy

This April 1996 image from Hubble shows the beautiful, eerie silhouette of dark dust clouds against the glowing nucleus of the elliptical galaxy NGC 1316. It may represent the aftermath of a 100 million-year-old cosmic collision between the elliptical and a smaller companion galaxy.
Mars

This image released Aug. 27, 2003, shows a close-up of the red planet Mars when it was just 34,648,840 miles away. The color image was assembled from a series of exposures. Many small, dark, circular impact craters can be seen, attesting to the Hubble telescope's ability to reveal fine detail on the planet's surface.
Hubble Space Telescope

The sun reflects off the newly installed solar panels of the Hubble Space Telescope as it sits in the cargo bay of the space shuttle Endeavour on Dec. 9, 1993.
Hubble Space Telescope

Jeff Rudolph, president of the California Science Center in Los Angeles, is photographed in front of a Hubble Space Telescope image of part of the Carina Nebula, a place in our galaxy where stars are born, at the California Science Center on Aug. 17, 2012.