Imagine the Universe! (2024)

Gamma-ray Detectors Introduction

Imagine the Universe! (1)

Photo of the Burst Alert Telescope (BAT) on NASA's Swift satellite under construction. (Credit: NASA/Swift)

Gamma rays, like visible light, are made up of packets of energy called photons. However, gamma-ray photons have millions of times more energy than visible light photons. At the same time, sources of cosmic gamma rays are extremely weak (that is, they produce relatively few gamma-ray photons for us to detect near Earth). Like X-ray detection, gamma-ray detection is done photon-by-photon.

Gamma rays are detected by observing the effects they have on matter. A gamma ray can collide with an electron and bounce off it like a billiard ball (Compton scatter) or it can push an electron to a higher energy level (photoelectric ionization). Also, since gamma rays have so much energy, part of this energy can be transformed into matter directly by creating an electron and another particle (called a pair production). All of these interactions cause electrons to move in some way, which basically means that an electric current has been created. These currents can then be amplified and measured to estimate the energy and direction of the original gamma-ray.

Gamma-ray detectors can be placed in two broad classes: spectrometers and imagers.

The first class would typically be called spectrometers or photometers in optical astronomy. These detectors are essentially "light buckets" that focus on a region of the sky containing the object of interest collecting as many photons as possible. These types of detectors generally use scintillators or solid-state detectors to transform the gamma-ray into optical or electronic signals that are recorded.

The second class are detectors which perform the difficult task of gamma-ray imaging. Detectors of this type either rely on the nature of the gamma-ray interaction process, such as pair production or Compton scattering, to calculate the arrival direction of the incoming photon, or they use a device such as a coded-mask to allow an image to be reconstructed.

Text updated: September 2018

Imagine the Universe! (2024)

FAQs

Imagine the Universe!? ›

If we were to shrink the Sun down to a grain of sand, then the observable Universe would only be a little over a hundred billion kilometers in radius, containing around 2 sextillion “grains of sand” (stars) strewn across that enormous volume.

How to imagine the size of the universe? ›

If we were to shrink the Sun down to a grain of sand, then the observable Universe would only be a little over a hundred billion kilometers in radius, containing around 2 sextillion “grains of sand” (stars) strewn across that enormous volume.

What are the three types of universe? ›

We will first consider the three most basic types. There are basically three possible shapes to the Universe; a flat Universe (Euclidean or zero curvature), a spherical or closed Universe (positive curvature) or a hyperbolic or open Universe (negative curvature).

What does the universe look like? ›

The observable universe is a ball-shaped region of the universe consisting of all matter that can be observed from Earth or its space-based telescopes and exploratory probes at the present time; the electromagnetic radiation from these objects has had time to reach the Solar System and Earth since the beginning of the ...

How big is our universe really? ›

The proper distance—the distance as would be measured at a specific time, including the present—between Earth and the edge of the observable universe is 46 billion light-years (14 billion parsecs), making the diameter of the observable universe about 93 billion light-years (28 billion parsecs).

How many universes are there? ›

The most exciting part of asking, “how many universes are there” is that there isn't a concrete answer yet. Multiverses are theoretically possible within our understanding of physics. It's highly unlikely that real alternate universes match most pop culture multiverses.

What is 42 in astrophysics? ›

In astrophysics, there is a curious coincidence involving the angle at which light from distant galaxies is bent due to gravitational lensing. This angle, known as the critical angle, is roughly 42 degrees for a standard cosmological model. The allure of 42 extends to philosophy and the human quest for meaning.

What is the biggest unsolved mystery of the universe? ›

Dark matter is the biggest unsolved mystery of the universe, and it could hold the key to understanding the origin, evolution, and fate of the cosmos. Until we find out what it is, we can only marvel at the dark side of the universe.

Are we alone in the universe? ›

Observations from the ground and from space have confirmed thousands of planets beyond our solar system. Our galaxy likely holds trillions. But so far, we have no evidence of life beyond Earth.

What's bigger than the universe? ›

The universe, being all there is, is infinitely big and has no edge, so there's no outside to even talk about. Oh, sure, there's an outside to our observable patch of the universe. The cosmos is only so old, and light only travels so fast.

What exists outside the universe? ›

This isn't a question that physics can answer with our present knowledge or without some form of qualification. The trite answer is that both space and time were created at the big bang about 14 billion years ago, so there is nothing beyond the universe.

What goes beyond the universe? ›

Outside the bounds of our universe may lie a "super" universe. Space outside space that extends infinitely into what our little bubble of a universe may expand into forever. Lying hundreds of billions of light years from us could be other island universes much like our own.

What universe is we in? ›

In the vast, expanding space known as the universe, humans reside on a small, rocky planet called Earth. Our planet is part of a discrete solar system in an arm of the spiral shaped Milky Way Galaxy. Our galaxy is only one of billions of other galaxies that exist within the universe.

Is it possible to comprehend the size of the universe? ›

After all that, I'll let you in on a secret: even astronomers can't truly grasp these scales. We work with them and we can do the math and physics with them, but our ape brain still struggles to comprehend even the distance to the moon—and the universe is 2 million trillion times bigger than that.

Why can't we understand the size of the universe? ›

The size of the Universe is difficult to determine because it is constantly expanding. However, current estimates put the observable Universe at around 93 billion light years in diameter.

Why is it so hard to tell the size of the universe? ›

That is because we can only see as far as light (or more accurately the microwave radiation thrown out from the Big Bang) has travelled since the Universe began. Since the Universe burst into existence an estimated 13.8 billion years ago, it has been expanding outwards ever since.

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