How can I judge exposure accurately on the camera LCD for night sky photos?

Asked 11/18/2014

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When shooting the night sky, I often dim the camera LCD so it doesn’t ruin my night vision. The problem is that photos can look fine on the camera, but later on my computer they turn out underexposed. If I raise the LCD brightness, I sometimes end up overexposing instead. What’s the best way to judge exposure in-camera for astrophotography, without relying on the LCD brightness alone?

Originally by Photography Stack Exchange contributor. Source · Licensed CC BY-SA 4.0

Photography Stack Exchange contributor

11y ago

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Read the histogram, not the image on the LCD.

In addition to errors because of screen brightness vs ambient brightness, the image on your screen is corrected by your camera before showing it on the screen. Most cameras allow you to adjust that, to remove saturation/sharpening adjustments, but you're still trying to judge your raw image based on an "edited" image on a tiny screen.

You need to read the histogram instead. The histogram is a graph of how much data you have at each brightness level. For stars, you're looking for a spike near, but not touching, the right side; an image that's mostly dark but has a few bright pixels.


Edit: I was on my phone earlier and totally botched my description of what the histogram should look like.

When reading a histogram, the exercise is left to the photographer to decide what information falls where on the brightness scale, and therefore how best to use the dynamic range of the camera. When photographing stars the important data is just a few bright pixels, which is not going to be easily spotted in the histogram. Most of the histogram will be dark pixels, and it's ok for them to be near or below the bottom of the histogram—there's no "shadows" to recover later in post processing. What you want to look out for, then, is a small spike on the right edge of the histogram, indicating clipped (lost) information. As a result, the histogram will look very unbalanced.

Here's an example of the lightroom histogram of one of my star shots, you can see it's skewed to the right so that there's no clipping of bright stars. I shot this under optimal conditions straight into the Milky Way, so the sky was bright enough that I was able to fit the entire dynamic range of the image into my camera's dynamic range (no clipping on either side). Full resolution here.

enter image description here

Technically I could have made my exposure slightly brighter to bring my histogram slightly closer to center and improve the tonal range in the darker, colored parts of the image, but with my equipment I did not want to push past ISO 3200 and after 15 seconds the stars would start to show motion blur.

Originally by user34574. Source · Licensed CC BY-SA 4.0

user34574

11y ago

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AI Answer

Generated from our catalog & community — verify before relying on it.

Don’t judge exposure by how the image looks on the LCD alone. LCD brightness and ambient darkness can mislead you, especially at night.

Use the histogram instead. It shows the distribution of tones in the image and is a much more reliable exposure guide than the preview screen. Also remember that the camera’s LCD preview is based on a processed JPEG-style rendering, not a perfect representation of the RAW file.

For night sky images, expect most of the frame to be dark, so the histogram will usually be weighted toward the left. The important part is to avoid clipping highlights if you want to preserve bright stars, and to make sure the data isn’t crushed unnecessarily.

In short: set the LCD to whatever brightness is comfortable for your eyes, but evaluate exposure with the histogram rather than the image preview.

UniqueBot

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11y ago

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