Sky Orientation through a Telescope

Looking through an eyepiece, the sky orientation will take on a different appearance depending on which type of telescope you use.

By Tim TrottStargazing For Beginners • June 8, 2014
Observational Astronomy

This article is part of a series of articles. Please use the links below to navigate between the articles.

  1. A Beginner's Guide To Observing The Night Sky - Stargazing!
  2. Tips for Improving Your Dark Eye Adaptation in Low Light Conditions
  3. Light Pollution and Dark Skies - Causes and Solutions
  4. How to Use Star Charts, Planispheres and Star Hopping
  5. Top Tips for Binocular Astronomy to See The Night Sky
  6. The Ultimate Guide to Moon Watching and Observing the Moon
  7. Tips for Buying Your First Telescope - What Type? How Big?
  8. What to Expect From Your First Night With Your First Telescope
  9. Sky Orientation through a Telescope
  10. Polar Alignment of an Equatorial Telescope Mount
  11. Everything You Wanted To Know About Telescope Eyepieces
  12. Which Astronomy Filters To Use For Astrophotography and Observation
  13. How to Photograph Constellations and Starry Nights
Sky Orientation through a Telescope

Looking through an eyepiece, the sky will take on a different orientation depending on your telescope. This is due to the telescope optics reflecting and refracting the light differently. Through some telescopes, night sky objects will appear upside down, back to front or simultaneously. Add the often confusing equatorial mount movement and tilt, and you'd be forgiven for thinking something was wrong.

Each telescope design has a different optical configuration, and these systems produce different views of the sky. With time, you get used to the way your telescope's optics work, just like you get used to your reflection in the mirror or using a rear-view mirror in the car. In these cases, our brains reverse the images without a second thought, and a telescope is no different.

Even though there is no "up" in astronomy, what is up in the northern hemisphere is down in the southern hemisphere; it is often comforting to correct things to what you are accustomed to. Not only does it bring objects back to their familiar orientation, but it also makes reading star charts and star hopping easier - when you are trying to star hop to a faint target under the glow of a red torch, revered images can be trying.

The difference in orientation is a consequence of how the light is brought to focus by each telescope design.

Newtonian Telescope Cutaway showing the focal length
Newtonian Telescope Cutaway showing the focal length

In general, if your telescope has an even number of elements - such as a Newtonian reflector, your target will appear upside down. The image is reversed from left to right if it has an odd number, such as a Nasmyth-Coude with its three-mirror configuration. A simple refracting telescope produces an upside-down view.

Changing face of the Moon

Moon Correctly Orientated
Moon Correctly Orientated
Moon up side down in Newtonian
Moon up side down in Newtonian
Moon upright and mirrored
Moon upright and mirrored
Moon upside down and mirrored
Moon upside down and mirrored

Correcting Sky Orientation

Fortunately, a few accessories use prism diagonals to solve this problem. They provide a correctly oriented view. Porro prisms (classical erecting prisms) provide correct images while allowing viewing straight through the scope.

Star Diagonals

45° Erecting Prism
45° Erecting Prism

Star diagonals work by adding a mirror angled at 45° into the light path. This bounces the light through 90° from the direction it entered the telescope, which has the effect of orientating the image so that it is the right way up but back to the front.

Erecting Eyepieces

These also reflect light through 90°, but they use prisms. They are sometimes sold with telescopes but are much more useful for terrestrial observation as the extra glass they contain dims the view of faint starlight.

Remember that when adding extra equipment between your telescope and your eye or camera, the image will become more degraded. You will lose light as optics scatter some away, and you may introduce aberrations to the image.

About the Author

Tim Trott is an avid stargazer and astrophotographer whose passion for the cosmos fuels a lifelong journey of exploration and wonder. Through Perfect Astronomy, he shares the beauty of the night sky and the art of capturing it, blending science and creativity to inspire curious minds and aspiring astrophotographers alike. Join him as he turns every starry night into a story waiting to be told.

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