A Manual to Accompany Software forthe Inductory Astronomy Lab ExerciseDocument SMG 8: Version 1Department of PhysicsGettysburg CollegeGettysburg, PA17325Telephone: (717) 337-6028email: [email protected]Contemporary LaboratoryExperiences in AstronomyRadio Astronomy of PulsarsStudent Manual
We have textbook solutions for you!

The document you are viewing contains questions related to this textbook.
ContentsGoals.....................................................................................................................................................3Objectives.............................................................................................................................................3Operating the Computer.......................................................................................................................6Starting the program.............................................................................................................................7Procedure..............................................................................................................................................7Part 1:The Radio Telescope........................................................................................................................................7Part 2:Observation of a Pulsar with a Single-Channel Radio Receiver.......................................................................8Part 3:The Periods of Different Pulsars......................................................................................................................11Part 4:Measurement of the Distance of Pulsars Using Dispersion............................................................................12A.Method...........................................................................................................................................................12B.An Example from the Everyday World..........................................................................................................12C.The Dispersion Formula for the Interstellar Medium.....................................................................................14D.Measuring The Distances Of Pulsars.............................................................................................................15Part 5: Determine the distance of Pulsar 2154+40 applying the techniques you have just learned. ...........................17Additional Exercises You Can Do With This Telescope.....................................................................181.The Distance To Short-Period Pulsars....................................................................................................................182.Measuring the Telescope Beamwidth.....................................................................................................................183.Measuring the Pulsar Spin-Down Rate...................................................................................................................194.Searching for Pulsars..............................................................................................................................................19
Version 1.0PAGE3GoalsYou should be understand the fundamental operation of a radio telescope and recognize how it issimilar to, and different from, an optical telescope. You should understand how astronomers, usingradio telescopes, recognize the distinctive properties of pulsars. You should understand what ismeant by interstellar dispersion, and how it enables us to measure the distances to pulsars.ObjectivesIf you learn to.......Use a simulated radio telescope equipped with a multi-channel receiver.Operate the controls of the receiver to obtain the best display of pulsar signals.Record data from these receivers.Analyze the data to determine properties of the pulsars such as periods, signal strengths atdifferent frequencies, pulse arrival times, relative strengths of the signals.Understand how the differences in arrival times of radio pulses at different frequencies tellus the distance the pulses have travel.You should be able to.....Understand the basic operation and characteristics of a radio telescope.Compare the periods of different pulsars, and understand the range of periods we find forpulsars.Understand how a pulsar’s signal strength depends on frequency.Determine the distance of several pulsars.Useful Terms You Should Review Using Your TextbookCrab Nebulainterstellar mediumpulsarfrequencyDeclinationJulian Dateradio telescopeparsecsdispersionmagnetic fieldradio wavesperiodelectromagnetic spectrumneutron starresolutionspeed of lightelectromagnetic radiationUniversal Time (UT)Right Ascension
Student ManualPAGE4Background: Neutron Stars and PulsarsMany of the most massive stars, astronomers believe, end their lives as neutron stars. These are bizarre objectsso compressed that they consist entirely of neutrons, with so little space between them that a star containing the mass ofour sun occupies a sphere no larger than about 10 km. in diameter, roughly the size of Manhattan Island. Such objects,
Upload your study docs or become a
Course Hero member to access this document
Upload your study docs or become a
Course Hero member to access this document
End of preview. Want to read all 21 pages?
Upload your study docs or become a
Course Hero member to access this document