Featured Resources
Classroom-Ready Activities
Science Olympiad Webinar
Science Olympiad JS9 Guide
Space Math @ NASA
NSO Tests 2025
- RFTS UTX Invitational Test
- UTX Astro Invitational
- UTX Astro Walkthrough
Informal Education
Background
Interactive Games
Space Scoop
STOP for Science
Chandra Podcasts
Printable Materials
Resource Request
Educators' Comments
Evaluation Form
Education Collaborations
Passport to Knowledge
Space Place
Web Shortcuts
Chandra Blog
RSS Feed
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information

Blasts From The Past: Historic Supernovas
Images

  Flash from Chandra.

Analyzing X-Ray Pulses from Stellar Cores - Answer Key:

GK Per

Power Spectrum (period confirmed with "period fold")
Frequency = 0.00285hz
Period = 351s

If white dwarf:

g = (6.67 x 10-11Nm2/kg2) (2.0x1030kg)/(6.4x106m)2 = 3.2x106m/s2

ac = (4π2) (6.4x106m)/(351s)2 = 2.1x103m/s2

ac is less than g – GK Per could sustain this period if it were a white dwarf.

CEN X-3

Power Spectrum (period confirmed with "period fold")
Frequency = 0.208hz
Period = 4.8s

If white dwarf:

g is the same as above for GK Per = 3.2x106m/s2

ac = (4π2) (6.4x106m)/(4.8s)2 = 1.7x107m/s2

ac is greater than g – Cen X-3 could not sustain this period if it were a white dwarf.

If neutron star:

g = (6.67 x 10-11Nm2/kg2) (4.0x1030kg)/(10000m)2 = 2.7x1012m/s2

ac = (4π2) (10000m)/(4.8s)2 = 1.7x104m/s2

ac is less than g – Cen X-3 could sustain this period if it were a neutron star.