Author Topic: Pulsar Discovery: Mystery Space Signals 50 Yrs Ago Changed Our View of Universe  (Read 401 times)

0 Members and 1 Guest are viewing this topic.

Offline Buster's Uncle

  • In Buster's Orbit, I
  • Ascend
  • *
  • Posts: 49279
  • €532
  • View Inventory
  • Send /Gift
  • Because there are times when people just need a cute puppy  Soft kitty, warm kitty, little ball of fur  A WONDERFUL concept, Unity - & a 1-way trip that cost 400 trillion & 40 yrs.  
  • AC2 is my instrument, my heart, as I play my song.
  • Planet tales writer Smilie Artist Custom Faction Modder AC2 Wiki contributor Downloads Contributor
    • View Profile
    • My Custom Factions
    • Awards
Pulsar Discovery: How Mystery Space Signals Recorded 50 Years Ago Changed Our View of the Universe
Newsweek
Simon Johnston  •November 28, 2017



This article was originally published on The Conversation. Read the original article.

A pulsar is a small, spinning star—a giant ball of neutrons, left behind after a normal star has died in a fiery explosion.

With a diameter of only 19 miles, the star spins up to hundreds of times a second, while sending out a beam of radio waves (and sometimes other radiation, such as X-rays). When the beam is pointed in our direction and into our telescopes, we see a pulse.

This year marks 50 years since pulsars were discovered. In that time, we have found more than 2,600 pulsars (mostly in the Milky Way), and used them to hunt for low-frequency gravitational waves, to determine the structure of our galaxy and to test the general theory of relativity.


The discovery

In mid-1967, when thousands of people were enjoying the “Summer of Love,” a young Ph.D. student at the University of Cambridge, in the United Kingdom, was helping to build a telescope.

It was a poles-and-wires affair—what astronomers call a “dipole array.” It covered a bit less than two hectares, the area of 57 tennis courts.

By July, it was completed. The student, Jocelyn Bell (now Dame Jocelyn Bell Burnell), became responsible for running it and analyzing the data it churned out. The data came in the form of pen-on-paper chart records, more than 100 feet of them each day. Bell analyzed them by eye.



Jocelyn Bell in 1967, the year she and her supervisor, Antony Hewish, discovered pulsars.   Roger W Haworth/Flickr


What she found—a little bit of “scruff” on the chart records—has gone down in history.

Like most discoveries, it took place over time. But there was a turning point. On November 28, 1967, Bell and her supervisor, Antony Hewish, were able to capture a “fast recording”—that is, a detailed one—of one of the strange signals.

In this she could see for the first time that the “scruff” was actually a train of pulses spaced by one-and-a-third seconds. Bell and Hewish had discovered pulsars.

But this wasn’t immediately obvious to them. Following Bell’s observation they worked for two months to eliminate mundane explanations for the signals.

Bell also found another three sources of pulses, which helped to scotch some rather more exotic explanations, such as the idea that the signals came from “little green men” in extraterrestrial civilizations. The discovery paper appeared in Nature on February 24, 1968.

Later, Bell missed out when Hewish and his colleague Sir Martin Ryle were awarded the 1974 Nobel Prize in Physics.



Astronomers using NASA’s Chandra X-ray Observatory found this pulsar, known as PSR J0357+3205 (or PSR J0357 for short). NASA handout image released on August 18, 2011. This year marks 50 years since pulsars were discovered.   NASA/Reuters


The Commonwealth Scientific and Industrial Research Organisation (CSIRO) Parkes radio telescope in Australia made its first observation of a pulsar in 1968, a sighting later memorialized (along with the Parkes telescope) on the first Australian $50 note.

Fifty years later, Parkes has found more than half of the known pulsars. The University of Sydney’s Molonglo Telescope has also played a central role. Both remain active in finding and timing pulsars today.

Internationally, one of the most exciting new instruments on the scene is China’s 500-meter (1,640 foot) Aperture Spherical Telescope, or FAST. It has recently located several new pulsars, confirmed by the Parkes telescope and a team of CSIRO astronomers working with their Chinese colleagues.


Why look for pulsars?

We want to understand what pulsars are, how they work and how they fit into the general population of stars. The extreme cases of pulsars—those that are superfast, super slow or extremely massive—help to focus the possible models for how pulsars work, telling us more about the structure of matter at ultrahigh densities. To find these extreme cases, we need to find lots of pulsars.

Pulsars often orbit companion stars in binary systems, and the nature of these companions helps us understand the formation history of the pulsars themselves. We’ve made good progress with the “what” and “how” of pulsars, but there are still unanswered questions.

As well as understanding pulsars themselves, we also use them as a clock. For example, pulsar timing is being pursued as a way to detect the background rumble of low-frequency gravitational waves throughout the universe.

Pulsars have also been used to measure the structure of our galaxy, by looking at the way their signals are altered as they travel through denser regions of material in space.

Pulsars are also one of the finest tools we have for testing Einstein’s theory of general relativity.



Albert Einstein in 1947. Einstein’s theory of relativity has survived 100 years of the most sophisticated tests astronomers have been able throw at it.   CC

This theory has survived 100 years of the most sophisticated tests astronomers have been able throw at it. But it doesn’t play nicely with our other most successful theory of how the universe works, quantum mechanics, so it must have a tiny flaw somewhere. Pulsars help us to try and understand this problem.

What keeps pulsar astronomers up at night (literally!) is the hope of finding a pulsar in orbit around a black hole. This is the most extreme system we can imagine for testing general relativity.

Finally, pulsars have some more down-to-earth applications. We’re using them as a teaching tool in our PULSE@Parkes program, in which students control the Parkes telescope over the internet and use it to observe pulsars. This program has reached over 1,700 students, in Australia, Japan, China, Netherlands, United Kingdom and South Africa.

Pulsars also offer promise as a navigation system for guiding craft traveling through deep space. In 2016, China launched a satellite, XPNAV-1, carrying a navigation system that uses periodic X-ray signals from certain pulsars.

Pulsars have changed our understanding of the universe, and their true importance is still unfolding.


http://www.newsweek.com/pulsars-50-anniversary-changed-view-universe-724268

 

* User

Welcome, Guest. Please login or register.
Did you miss your activation email?


Login with username, password and session length

Select language:

* Community poll

SMAC v.4 SMAX v.2 (or previous versions)
-=-
24 (7%)
XP Compatibility patch
-=-
9 (2%)
Gog version for Windows
-=-
103 (32%)
Scient (unofficial) patch
-=-
40 (12%)
Kyrub's latest patch
-=-
14 (4%)
Yitzi's latest patch
-=-
89 (28%)
AC for Mac
-=-
3 (0%)
AC for Linux
-=-
6 (1%)
Gog version for Mac
-=-
10 (3%)
No patch
-=-
16 (5%)
Total Members Voted: 314
AC2 Wiki Logo
-click pic for wik-

* Random quote

As the Americans learned so painfully in Earth's final century, free flow of information is the only safeguard against tyranny. The once-chained people whose leaders at last lose their grip on information flow will soon burst with freedom and vitality, but the free nation gradually constricting its grip on public discourse has begun its rapid slide into despotism. Beware of he who would deny you access to information, for in his heart he dreams himself your master.
~Commissioner Pravin Lal 'U.N. Declaration of Rights'

* Select your theme

*
Templates: 5: index (default), PortaMx/Mainindex (default), PortaMx/Frames (default), Display (default), GenericControls (default).
Sub templates: 8: init, html_above, body_above, portamx_above, main, portamx_below, body_below, html_below.
Language files: 4: index+Modifications.english (default), TopicRating/.english (default), PortaMx/PortaMx.english (default), OharaYTEmbed.english (default).
Style sheets: 0: .
Files included: 45 - 1228KB. (show)
Queries used: 36.

[Show Queries]