HomeNASANASA — Journey to Unique Locations in our Galaxy!

NASA — Journey to Unique Locations in our Galaxy!

Completed quadrant of an X-ray Mirror Assembly, under development for the JAXA/NASA XRISM mission. It is shaped like a fan with thin metal struts holding it together.ALT

Does the thing on this picture seem like a mirror? Perhaps not, however that’s precisely what it’s! To be extra exact, it’s a set of mirrors that might be used on an X-ray telescope. However why does it look nothing just like the mirrors you’re conversant in? To reply that, let’s first take a step again. Let’s discuss telescopes.

How does a telescope work?

The essential operate of a telescope is to assemble and focus gentle to amplify the sunshine’s supply. Astronomers have used telescopes for hundreds of years, and there are a couple of completely different designs. As we speak, most telescopes use curved mirrors that enlarge and focus gentle from distant objects onto your eye, a digital camera, or another instrument. The mirrors will be created from quite a lot of supplies, together with glass or metallic.

Diagram showing a reflecting telescope with a pair of mirrors to focus the light on the detector — in this case, an observer’s eye. The diagram shows the “flow” of light, which starts at a distant galaxy, enters the telescope and bounces off the primary mirror at the bottom of the telescope. Then the light moves to the secondary mirror which redirects the light out of the side of the telescope tube into the observer’s eye.ALT

Area telescopes just like the James Webb and Hubble Area Telescopes use giant mirrors to focus gentle from a number of the most distant objects within the sky. Nevertheless, the mirrors should be tailor-made for the kind and vary of sunshine the telescope goes to seize—and X-rays are particularly laborious to catch.

X-rays versus mirrors

X-rays are likely to zip by most issues. It is because X-rays have a lot smaller wavelengths than most different forms of gentle. In actual fact, X-rays will be smaller than a single atom of virtually each ingredient. When an X-ray encounters some surfaces, it might probably move proper between the atoms!

X-ray image of a human elbow. Denser materials, like bone, stop more X-rays than skin and muscle.ALT

Medical doctors use this property of X-rays to take photos of what’s inside you. They use a beam of X-rays that principally passes by pores and skin and muscle however is essentially blocked by denser supplies, like bone. The shadow of what was blocked reveals up on the movie.

This tendency to move by issues consists of most mirrors. In case you shoot a beam of X-rays into an ordinary telescope, a lot of the gentle would go proper by or be absorbed. The X-rays wouldn’t be centered by the mirror, and we wouldn’t be capable of examine them.

Animation first showing a plane of balls face-on and an arrow passing through the space between the balls. Then the angle changes to show the balls edge-on and an arrow bouncing off the top.ALT

X-rays can bounce off a specifically designed mirror, one turned on its facet in order that the incoming X-rays arrive nearly parallel to the floor and look off it. At this shallow angle, the area between atoms within the mirror’s floor shrinks a lot that X-rays can’t sneak by. The sunshine bounces off the mirror like a stone skipping on water. The sort of mirror is named a grazing incidence mirror.

A metallic onion

Telescope mirrors curve in order that all the incoming gentle involves the identical place. Mirrors for many telescopes are based mostly on the identical 3D form — a paraboloid. You would possibly keep in mind the parabola out of your math lessons because the cup-shaped curve. A paraboloid is a 3D model of that, spinning it across the axis, a little bit just like the nostril cone of a rocket. This seems to be an important form for focusing gentle at a degree.

A line drawing of a parabola - a cup-shaped curve, shown here on its side - spins around to create a 3D shape. The word “paraboloid” shows on the screen. Then part of the curve fades away, leaving behind two things:  a small concave circle, which was one end of the paraboloid, labeled “Radio dishes; optical, infrared and ultraviolet telescope mirrors,” and a cylinder with sloping walls, which was the part of the edges of the paraboloid, labeled “X-ray mirrors.”ALT

Mirrors for seen and infrared gentle and dishes for radio gentle use the “cup” portion of that paraboloid. For X-ray astronomy, we minimize it a little bit in another way to make use of the wall. Identical form, completely different piece. The mirrors for seen, infrared, ultraviolet, and radio telescopes seem like a gently-curving cup. The X-ray mirror seems like a cylinder with very barely angled partitions.

The picture under reveals how completely different the mirrors look. On the left is among the Chandra X-ray Observatory’s cylindrical mirrors. On the correct you’ll be able to see the gently curved spherical main mirror for the Stratospheric Observatory for Infrared Astronomy telescope.

On the left, a technician stands next to a cylinder-shaped mirror designed for X-ray astronomy. The mirror is held in a frame a little off the ground, and is about as tall as the technician. On the right, two technicians inspect a round mirror for optical astronomy.ALT

If we use only one grazing incidence mirror in an X-ray telescope, there can be an enormous gap, as proven above (left). We’d miss lots of X-rays! As a substitute, our mirror makers fill in that cylinder with layers and layers of mirrors, like an onion. Then we will gather extra of the X-rays that enter the telescope, giving us extra gentle to review.

Completed X-ray Mirror Assembly for the X-ray Imaging and Spectroscopy Mission (XRISM, pronounced “crism”), which is a collaboration between the Japan Aerospace Exploration Agency (JAXA) and NASA, along with ESA participation. The assembly has thin metal struts fanning outward from a silver ring in the center of the image. Shiny ridge surfaces (actually many thin mirrors!) fill in the spaces between the struts.ALT

Nested mirrors like this have been utilized in many X-ray telescopes. Above is a close-up of the mirrors for an upcoming observatory known as the X-ray Imaging and Spectroscopy Mission (XRISM, pronounced “crism”), which is a Japan Aerospace Exploration Company (JAXA)-led worldwide collaboration between JAXA, NASA, and the European Area Company (ESA).

The XRISM mirror meeting makes use of skinny, gold-coated mirrors to make them tremendous reflective to X-rays. Every of the 2 assemblies has 1,624 of those layers packed in them. And every layer is so easy that the roughest spots rise no a couple of millionth of a millimeter.

Chandra observations of the Perseus galaxy cluster showing turbulence in the hot X-ray-emitting gas.ALT

Why go to all this bother to gather this elusive gentle? X-rays are an effective way to review the most well liked and most energetic areas of the universe! For instance, on the facilities of sure galaxies, there are black holes that warmth up fuel, producing every kind of sunshine. The X-rays can present us gentle emitted by materials simply earlier than it falls in.

Keep tuned to NASA Universe on Twitter and Fb to maintain up with the most recent on XRISM and different X-ray observatories.

Ensure to comply with us on Tumblr to your common dose of area!



Please enter your comment!
Please enter your name here

Most Popular

Recent Comments