AstronomyOnline.org
home observation science solar system stars our galaxy cosmology astrobiology exoplanets astrophotography
Science
icon Introduction
icon Astronomy Tools
Concepts
1. Electromagnetic Spectrum
2. Atmosphere Limitations
3. Space Observations
Equipment
1. Telescopes
2. Radio
3. Space Tools
4. Photography
5. Spectroscopy
6. Computers
7. Advanced Methods
8. Radio Astronomy
icon Basic Mathematics
Algebra
Statistics
Geometry
Scientific Notation
Log Scales
Calculus
icon Physics
Concepts
- Basic Units of Measure
- Mass & Density
- Temperature
- Velocity & Acceleration
- Force, Pressure & Energy
- Atoms
- Quantum Physics
- Nature of Light
Formulas
- Brightness
- Cepheid Rulers
- Distance
- Doppler Shift
- Frequency & Wavelength
- Hubble's Law
- Inverse Square Law
- Kinetic Energy
- Luminosity
- Magnitudes
- Convert Mass to Energy
- Kepler & Newton - Orbits
- Parallax
- Planck's Law
- Relativistic Redshift
- Relativity
- Schwarzschild Radius 
- Synodic & Sidereal Periods
- Sidereal Time
- Small Angle Formula
- Stellar Properties 
- Stephan-Boltzmann Law
- Telescope Related
- Temperature
- Tidal Forces
- Wien's Law
Constants
icon Computer Models
icon Additional Resources
1. Advanced Topics
2. Guest Contributions
Physics - Formulas - Parallax

Our abilities as humans to determine distance to an object is a result of the brains process of visual data. Both our eyes work in tandem to that any shift from one eye to another allows for a determination of distance. This is called parallax, or change in an objects position based on the point of view of the observer. The same effect works in stars (that are nearby only). This effect can be measured:

One of the nearby stars is Barnard's Star. It has a parallax angle of 0.547 arcseconds. To find the distance:

Back to Top

 

Search | Site Map | Appendix
©2004 - 2024 Astronomy Online. All rights reserved. Contact Us. Legal. Creative Commons License
The works within is licensed under a Creative Commons Attribution-ShareAlike 3.0 Unported License.