Radio_Astronomy_pre-lab_03-23-10 - Radio Astronomy of...

Info iconThis preview shows pages 1–2. Sign up to view the full content.

View Full Document Right Arrow Icon
Radio Astronomy of Pulsars Pre-lab Introduction to Pulsars Many of the most massive stars, astronomers believe, end their lives as neutron stars. These are bizarre objects so compressed that they consist mainly of neutrons, with so little space between them that a star containing the mass of our sun occupies a sphere no larger than about 10 km. in diameter, roughly the size of Manhattan Island. Such objects, one would think, would be extremely hard, if not impossible, to detect. Their surface areas would be several billion times smaller than the sun, and they would emit so little energy (unless they were impossibly hot) that they could not be seen over interstellar distances. Astronomers were therefore quite surprised to discover short, regular bursts of radio radiation coming from neutron stars—in fact it took them a while before they realized what it was they were seeing. The objects they discovered were called pulsars, which is short for “pulsating radio sources.” The discovery of pulsars was made quite by accident. In 1967, Jocelyn Bell, who working for her Ph.D. under Anthony Hewish in Cambridge, England, was conducting a survey of the heavens with a new radio telescope that was designed specifically to look for rapid variations in the strengths of signals from distant objects. The signals from these objects varied rapidly in a random fashion due to random motions in the interstellar gas they pass through on their way to earth, just as stars twinkle randomly due to motions of air in the earth’s atmosphere. Bell was surprised one evening in November, 1967 to discover a signal that varied regularly and systematically , not in a random fashion. It consisted of what looked like an endless series of short bursts of radio waves, evenly spaced precisely 1.33720113 seconds apart. The pulses were so regular, and so unlike natural signals, that, for a while, Bell and Hewish tried to find some artificial source of radiation—like a radar set or home appliance—that was producing the regular interference. It soon became clear that the regular pulses moved across the sky like stars, and so they must be coming from space. The astronomers even entertained the idea that they were coming from “Little Green Men” who were signaling to the earth. But when three
Background image of page 1

Info iconThis preview has intentionally blurred sections. Sign up to view the full version.

View Full DocumentRight Arrow Icon
Image of page 2
This is the end of the preview. Sign up to access the rest of the document.

This note was uploaded on 02/06/2011 for the course ASTR 114 taught by Professor Staff during the Spring '08 term at George Mason.

Page1 / 3

Radio_Astronomy_pre-lab_03-23-10 - Radio Astronomy of...

This preview shows document pages 1 - 2. Sign up to view the full document.

View Full Document Right Arrow Icon
Ask a homework question - tutors are online