Ora

How do you align a telescope to Polaris?

Published in Telescope Alignment 5 mins read

Aligning a telescope to Polaris is a fundamental step for observers in the Northern Hemisphere using an equatorial mount, crucial for accurate tracking of celestial objects across the night sky.

Understanding Polar Alignment

Polar alignment is the process of precisely orienting the rotational axis of your telescope mount to be parallel with Earth's rotational axis. This allows your telescope to track stars and other celestial objects by moving along only one axis (the Right Ascension axis), simplifying observation and enabling long-exposure astrophotography without star trails.

For Northern Hemisphere observers, Polaris, commonly known as the North Star, is the key to this alignment because it is located very close to the North Celestial Pole (NCP), the point in the sky directly above Earth's rotational axis.

Essential Tools for Polaris Alignment

A successful polar alignment relies on having the right equipment and understanding its function.

Tool Purpose
Equatorial Mount The specific type of mount designed for polar alignment and celestial tracking.
Finderscope A small, wide-field scope attached to your main telescope, often with a reticle.
Polar Scope (Optional, but highly recommended for precision) A specialized scope integrated into the mount's Right Ascension axis.
Star Chart/App To accurately locate Polaris in the night sky.
Spirit Level To ensure your tripod is perfectly level, a critical starting point.
Mount Adjustment Knobs For fine-tuning altitude (latitude) and azimuth (left-right) adjustments.

Step-by-Step Guide to Aligning Your Telescope to Polaris

Achieving accurate polar alignment involves several steps, from initial setup to fine-tuning.

Initial Setup and Preparation

  1. Set Up Your Mount: Place your equatorial mount on stable, level ground. Ensure the tripod legs are fully extended and firmly planted.
  2. Level the Tripod: Use a spirit level to ensure your tripod head is perfectly level. This is crucial for accurate altitude adjustments later.
  3. Roughly Point North: Orient your mount's Right Ascension (RA) axis roughly towards true north. Many mounts have an indicator or an opening for a polar scope that should point North.
  4. Set Your Latitude: Adjust your mount's altitude (or latitude) setting to match your geographical latitude. There's usually a scale on the mount for this. This gets you close to the correct elevation for the celestial pole.
  5. Balance Your Telescope: Properly balance your telescope on the mount. This prevents strain on the motors and ensures smooth tracking.

Locating Polaris

For observers in the Northern Hemisphere, locating Polaris is the first visual step.

  • Use a Star Chart or Astronomy App: Utilize a reliable star chart or a modern astronomy app (like SkyView Lite or Stellarium Mobile) on your smartphone to precisely identify Polaris. It is the end star of the Little Dipper's handle and can also be found by following a line from the two pointer stars of the Big Dipper.

Rough Alignment using the Finderscope

This initial alignment step is critical for getting Polaris into view.

  1. Set Declination: Ensure the declination setting circle on your mount reads 90 degrees. This aligns your telescope tube with the polar axis of the mount.
  2. Adjust the Mount: Without moving the main telescope tube, you will adjust the entire mount using its azimuth (left/right) and altitude (up/down) adjustment knobs. The goal is to center Polaris in the reticle of your finderscope.
  3. Do NOT Move the Telescope Tube: It is essential during this step that you do not move the telescope tube relative to the mount's axes. All adjustments must come from the mount itself.

Fine Alignment (Using a Polar Scope for Precision)

For astrophotography or very long observation sessions, a polar scope provides greater accuracy.

  1. Access the Polar Scope: If your mount has a polar scope, remove any covers or caps to look through it.
  2. Align the Reticle: The polar scope will have a specialized reticle (a pattern of circles or a small dipper shape). Polaris is not exactly at the North Celestial Pole; it orbits it in a small circle. You need to rotate the polar scope's reticle to match the current orientation of the constellation it depicts (often the Little Dipper) relative to the sky. Many polar scopes have markings to help you place Polaris in its correct offset position for the current time and date. Apps like PolarFinder or built-in functions in telescope control apps can help you determine Polaris's exact position on the reticle.
  3. Adjust Mount Again: Using the mount's altitude and azimuth fine-adjustment knobs, move the entire mount until Polaris is positioned correctly within the polar scope's reticle according to its current offset.

Tips for Accurate Polar Alignment

  • Prioritize Leveling: A perfectly level tripod simplifies all subsequent adjustments significantly.
  • Balance Your Scope: An unbalanced scope can cause "wobbles" or "jerks" during tracking, even with perfect alignment.
  • Clear View: Ensure your polar scope is clean and focused for the sharpest view of Polaris.
  • Practice Makes Perfect: Polar alignment can seem daunting at first, but with practice, it becomes a quick and routine setup.
  • Use Drift Alignment for Utmost Precision: For highly demanding astrophotography, a technique called "drift alignment" can refine your polar alignment beyond what a polar scope can achieve. This involves observing how a star near the celestial equator drifts in declination.

Common Misconceptions

  • Polaris is exactly at the Celestial Pole: Polaris is very close, but not precisely at the North Celestial Pole. It currently lies about 0.6 degrees away, meaning it traces a small circle around the true pole each day. This offset is why polar scopes have special reticles.
  • Polar Alignment is the Same as GoTo Alignment: GoTo alignment (aligning to two or three bright stars) calibrates your telescope's computer to know its current orientation and time for accurate pointing. Polar alignment is about orienting the mount's axis itself, which is a prerequisite for GoTo systems on equatorial mounts to track accurately.