Observing Techniques

Seeing and Transparency are values that an observer uses to compare the quality of the sky from night to night. The values are very specific to an individual observer's visual acuity. Seeing is a measure of how stable the sky is. Transparency is a measure of how clear the sky is. Most of the Astronomical League's Observing Programs require the observer to evaluate these conditions for each observation and to record them in their observation log.

Here are two scales that are acceptable for all Observing Programs. They are simple to use and require no special equipment. Both of these values can be done very formally using special equipment, but for the TVS Observing Programs this level of effort is not required.

Seeing: How Stable is the sky?

Transparency: How clear is the sky?

Transparency is a measure of what you can see in the nighttime sky in spite of dust, smoke, haze, humidity, or light pollution. An easy way to measure this is to use the magnitude of the faintest star you can see. Ideally, this would be looking straight up at zenith. But, to make life simpler, you can use the Little Dipper (Ursa Minor) if you can see it. Here is the scale:
  1. If you can't see Polaris
  2. If you can only see Polaris
  3. If you can see the two stars on the end of the bowl of the Little Dipper (Kochab and Pherkad)
  4. If you can see any of the stars in the handle of the Little Dipper
  5. If you can see 6 of the 7 stars in the Little Dipper
  6. If you can see all 7 stars in the Little Dipper
  7. If you can see stars near the Little Dipper that are not part of the stick figure. (I envy your young eyes...)
Although atmospheric extinction will vary from season to season, and from latitude to latitude, using the Little Dipper is a simple and reasonable solution.