The Globe and Mail article The image below shows a telescope’s optics.

The image above shows the sky in the morning.

Both images are taken by the Very Large Telescope in Chile.

The telescope was built in 1964 by the National Astronomical Observatory of Chile, and is about 3.2 kilometres (2.5 miles) across.

The view from the north is a bit dimmer than from the south.

If you want to see what it looks like in the dark, you’ll need a telescope of about the same size.

The first telescope was a 2-metre (6-foot) telescope.

The second telescope was bigger and longer, and has been used to look for signals from the Big Bang.

The third telescope, built in 1996, has a 3-metres (10-foot-wide) aperture.

The fourth telescope was an 11-meters (36-foot), 10-meter (30-foot-) diameter telescope.

And the fifth telescope is the longest and largest.

The five telescopes are the largest telescopes on the planet, but they’re still dwarfed by other large observatories.

“This is what you’d expect,” says Mark Hensley, an astrophysicist at the University of British Columbia in Vancouver.

“They’re dwarfed,” Hensleys says.

“The five telescopes in the constellation of Boötes, in the southern sky, are very small, but you can still see them because they’re so far away.”

Astronomers have been looking for signals of the Big Dipper for decades, but the telescope that we’re looking at now, built by the European Southern Observatory in Chile, has only recently begun to look at them.

“You can see the Big dipper just like you can see a star, or the moon, or a galaxy,” says Hensleys.

“It’s just that you can actually see it from this distance.”

What are the Big Observatories looking for?

The telescopes can observe the Big Dot, or star cluster, which contains about 1,000 stars.

The Big Observatory can also observe a cluster of stars called a red dwarf.

“These are the brightest stars in the galaxy that have not yet been found, so they’re very important,” Hinsley says.

In addition to looking for stars, astronomers also look for dark matter, which is the dark matter that makes up the matter of stars.

This dark matter contains about a third of the mass of the sun, and it’s thought to be a major force in the universe.

Astronomers can’t see it directly, but scientists can make predictions about how this dark matter will interact with the stars in a star cluster.

Astronomer Robert Green, of the University at Albany in New York, says that there are a couple of things astronomers can look for.

“One is the number of these stars, the brightness of these, the number in the cluster,” he says.

If there are many of these red dwarf stars in one cluster, that suggests a cluster is undergoing an evolution, Green says.

Another sign of a cluster’s evolution is the cluster’s alignment with other clusters.

This is called a merger, and when two or more stars are in the same place at the same time, they merge into one.

This means that one star is brighter than the other, but it also means the cluster is more crowded.

The cluster is thought to have been formed about 13 billion years ago, but there are other clusters that are closer to our solar system than that, such as the Andromeda galaxy.

The Andromeda galaxy is thought, in part, to have formed when the Andromeda Galaxy was one of a handful of smaller galaxies that were merged into a larger one.

“A galaxy like Andromeda would be very different from other galaxies,” Green says, because it’s surrounded by other galaxies.

Astronomical observations can also tell us whether a cluster contains stars.

Astronomy professor Michael J. Oster of the California Institute of Technology in Pasadena, California, says it’s not unusual for astronomers to look through a telescope and see bright, white light.

“But if you have a lot of stars, then you’ll see a lot more white light, as well,” he explains.

If the stars are so bright, and if the cluster looks like it’s being disrupted by other stars, there could be a lot going on, Oster says.

Astronaut Mark Kelly says that astronomers can see star clusters through telescopes.

Astronauts on the International Space Station watch the sky with their binoculars and use binocular lenses.

Astronom Michael Hays, of Columbia University, says observing a cluster through telescopes is a very simple way to observe the stars, because we can see them from space.

“If you look through the telescope, you can’t tell the difference between a star and a white dwarf,” he said.

The Astronomical Observatories of Japan has a telescope that can see stars through the binocular and sees them