·13 min read·By ExifGrabber Editorial Team

How to Edit Milky Way Photos in Lightroom and Photoshop: Complete Workflow

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The Milky Way galactic core above the ESO 3.6-metre telescope at La Silla Observatory
ESO/S. Brunier · CC BY 4.0

Why Milky Way Photos Need Editing

A Milky Way photo straight out of camera almost never looks like the final images you see online. High ISO noise muddies the stars. The white balance is usually wrong because your camera's auto white balance has no idea what to do with a dark sky full of stars. The Galactic Core looks washed out. Light pollution adds color casts. And the dynamic range between a bright Milky Way band and a dark foreground landscape is often more than a single exposure can handle gracefully.

The good news is that with a solid editing workflow, you can bring out the structure, color, and drama that your camera sensor actually captured. You don't need to fabricate anything. You're revealing what's already in the data. This guide walks through the entire process from RAW import to final export, using Adobe Lightroom and Photoshop.

If you're still working on capturing Milky Way images in the field, start with our beginner's guide to astrophotography and our guide to the best lenses for Milky Way photography. Once you have your RAW files, come back here.

Before You Start: Check Your RAW Files

Open your image in ExifGrabber to check the EXIF metadata. You want to confirm a few things before diving into edits.

ISO: Milky Way shots are typically at ISO 1600 to 6400. Higher ISOs mean more noise, which changes how aggressively you should apply noise reduction. Exposure time: Check that your shutter speed followed the 500 rule (or NPF rule) to avoid star trails. If stars are elongated, you may still be able to use the image, but it limits how far you can crop or enlarge. Focal length: Wider lenses (14-24mm) capture more sky but the Milky Way appears smaller. Longer focal lengths (35-50mm) require panoramic stitching but give more detail in the Galactic Core. White balance: Note the as-shot white balance. You'll override this in Lightroom, but it's useful to see where the camera started.

Step 1: Import and Initial Lightroom Setup

Import your RAW file into Lightroom Classic. Before touching any sliders, make two changes in the Develop module.

Set the profile to Adobe Standard. Click the Profile dropdown at the top of the Basic panel and select Adobe Standard (or Adobe Standard v2 if available). Camera-specific profiles (like Camera Landscape or Camera Vivid) apply aggressive processing that can create artifacts in night sky images.

Reset the Detail panel. Lightroom applies default sharpening (Amount: 40) and no noise reduction. For Milky Way work, set Sharpening Amount to 0 for now. You'll apply targeted sharpening later. Leaving the default on while making contrast and color adjustments amplifies noise at every step.

Step 2: White Balance

White balance is the single most impactful adjustment for a Milky Way image. The "correct" white balance for a night sky is debatable, but a temperature between 3800K and 4200K generally produces a natural-looking sky with good separation between the warm tones of the Galactic Core and the cooler surrounding sky.

Start at 3900K and adjust by eye. You want the sky background to appear a neutral dark gray, not blue and not orange. The Milky Way band itself should show a subtle warm tone, and the interstellar dust lanes should appear reddish-brown.

Tint usually needs a slight push toward magenta (+5 to +15) to counteract the green cast from airglow, which is a faint atmospheric emission that shows up in long exposures even from dark sky sites.

Avoid making the sky too blue. A common beginner mistake is cooling the white balance dramatically because a deep blue sky "looks right" on screen, but it crushes the subtle warm colors in the Milky Way's core and makes the image look monochromatic.

Step 3: Exposure and Tone

Work through the Basic panel tone sliders in this order.

Exposure: Adjust to taste, typically +0.3 to +0.7 stops. You want the overall image brighter without clipping the stars. Watch the histogram and make sure the right edge doesn't pile up.

Highlights: Pull to -50 to -80. This recovers detail in the brightest star clusters and the Milky Way core.

Shadows: Push to +40 to +70. This brings up the foreground landscape and the darker nebulae in the sky. Don't overdo it, as pushing shadows too far amplifies noise aggressively.

Whites: Set between +10 and +30. This adds a subtle brightness pop to the stars without the broad effect of the Exposure slider.

Blacks: Set between -10 and -30. This deepens the darkest parts of the sky, adding contrast and making the Milky Way stand out more. If your sky has light pollution gradients, be conservative here.

Contrast: Keep this low or at zero. You'll add contrast more precisely with other tools. The global Contrast slider is too blunt for astrophotography.

Step 4: Presence Sliders

The Presence sliders (Texture, Clarity, Dehaze) are where the Milky Way really starts to pop.

Texture: +20 to +40. Texture enhances fine detail without adding the halos that Clarity can introduce. It brings out the dust lanes and nebulae structure in the Milky Way.

Clarity: +20 to +50. Clarity increases midtone contrast, which adds depth and dimensionality to the Milky Way. Be careful above +50 because it can make the image look crunchy and amplifies noise.

Dehaze: +15 to +40. Dehaze is powerful for Milky Way images. It adds contrast and saturation simultaneously, cutting through the haze effect of light pollution and airglow. But it's the slider most likely to create an over-processed look, so use restraint. A common starting point is +25.

Step 5: Tone Curve

Switch to the Tone Curve panel and use the Point Curve for precise control.

Create a gentle S-curve: lift the shadows slightly (don't crush the blacks completely) and push the upper midtones. The key adjustment is pulling the bottom-left point of the curve up just slightly from the corner. This lifts the absolute blacks and prevents the sky from going to pure black, which looks more natural and reveals faint nebulosity.

If you want more contrast in the Milky Way core specifically, steepen the middle portion of the curve. A subtle S-curve goes a long way. Aggressive curves create banding artifacts in the smooth gradient areas of the night sky.

Step 6: HSL and Color

Open the HSL/Color panel. This is where you fine-tune the colors in your night sky.

Hue: Shift the Blue hue toward Aqua (-10 to -20) to counteract the tendency of night skies to go electric blue. Shift Orange slightly toward Yellow to warm up the Galactic Core.

Saturation: Increase Orange and Yellow saturation (+15 to +25) to bring out the warm tones of the Galactic Core. Increase Purple and Magenta slightly (+10 to +15) to enhance the nebula regions. Be conservative with Blue saturation because over-saturating blue skies looks artificial quickly.

Luminance: Decrease Blue luminance (-10 to -20) to darken the sky background. This makes the Milky Way pop more without adding contrast globally. Increase Orange luminance slightly to brighten the Galactic Core.

Step 7: Local Adjustments with Masks

Lightroom's masking tools let you apply targeted edits to specific areas. This is where you separate a good Milky Way edit from a great one.

Sky mask

Use Select Sky (Lightroom's AI masking) or paint a manual mask over the sky. Apply these adjustments to the sky only: a small boost to Clarity (+15), Dehaze (+10), and Texture (+10), plus a slight increase in Contrast (+15). This enhances the Milky Way without affecting the foreground landscape.

Galactic Core mask

Create a second mask targeting just the brightest part of the Milky Way. Use a large, feathered brush. Apply: Exposure +0.2, Clarity +10, Saturation +10. This draws the viewer's eye to the most dramatic part of the sky.

Foreground mask

If your foreground is a landscape, create a mask for it. You'll likely need to increase Exposure more than the sky, plus add Shadows (+30) and a touch of Warmth to separate it from the cooler sky tones.

Step 8: Noise Reduction

Noise reduction is the most consequential decision in Milky Way processing. Too little, and the image looks gritty. Too much, and the stars smear into soft blobs and the Milky Way loses its fine structure.

Lightroom's built-in noise reduction

In the Detail panel, start with Luminance noise reduction at 20-30 for ISO 3200 images, or 30-45 for ISO 6400+. Keep the Detail slider at 50 (default) and the Contrast slider at 0.

For Color noise reduction, the default (25) is usually sufficient. If you see colored speckling, increase to 40-50.

Lightroom's AI Denoise (available in recent versions) is significantly better than the traditional sliders for astrophotography. Use it at a strength of 40-60 for a good balance between noise removal and detail preservation. It processes the image as a new DNG, which you can then continue editing.

Image stacking (the superior method)

If you shot multiple identical exposures in the field (10-20 frames), stacking them before editing produces dramatically cleaner results than any single-frame noise reduction. The math is simple: stacking N frames reduces noise by a factor of roughly the square root of N. So 16 stacked frames give you 4x less noise than a single frame.

For stacking, use Sequator on Windows or Starry Landscape Stacker on Mac. These tools align the stars across frames (accounting for sky rotation), stack the sky, and separately stack the foreground (which doesn't rotate), then blend the two halves together.

For more on stacking and advanced astrophotography noise reduction, see our intermediate astrophotography guide.

Step 9: Sharpening

After noise reduction, apply sharpening selectively. Go back to the Detail panel.

Amount: 60-80 for a stacked image, 40-60 for a single frame (higher values amplify any remaining noise). Radius: 1.0 to 1.2. This works well for stars and fine nebula detail. Detail: 40-60. Higher values sharpen finer detail but also sharpen noise. Masking: Hold Alt/Option and drag the Masking slider until only the stars and bright Milky Way structure are white. This prevents sharpening the smooth, dark sky areas where it would only amplify noise. A Masking value of 60-80 works well for most Milky Way images.

Step 10: Moving to Photoshop

For many Milky Way images, the Lightroom adjustments above are sufficient. But Photoshop unlocks more advanced techniques, especially for sky/foreground blending and targeted enhancements.

Right-click your image in Lightroom and choose Edit In > Adobe Photoshop. This sends a 16-bit TIFF to Photoshop with your Lightroom adjustments baked in.

Sky and foreground blending

If you shot separate exposures for the sky and foreground (a common technique for balanced exposure), Photoshop's layer masks let you blend them seamlessly.

  1. Open both images as layers in Photoshop (File > Scripts > Load Files into Stack).
  2. Align the layers if needed (Edit > Auto-Align Layers).
  3. Add a layer mask to the top layer.
  4. Use a soft black brush (hardness 0%, flow 10-15%) to paint along the horizon, blending the sky from one exposure with the foreground from the other.
  5. Use a gradient on the mask for a smooth transition. Start the gradient just below the horizon line.

Selective color enhancement with curves

Photoshop's Curves adjustment layers give you per-channel control that's more precise than Lightroom's HSL sliders.

Create a Curves adjustment layer and switch to the Red channel. Add a subtle S-curve to increase contrast in the reds, which enhances the warm nebula regions. Do the same in the Blue channel with an inverted S-curve to reduce blue in the shadows (which deepens the sky) while maintaining it in the highlights (which keeps the cooler star colors).

Dodge and burn

Create a new layer set to Overlay blend mode and fill with 50% gray. Use a soft white brush at 5-10% opacity to paint (dodge) over the brightest parts of the Milky Way core. Use a soft black brush at the same opacity to darken (burn) the sky around the Milky Way, increasing the contrast between the band and the surrounding sky. This manual approach gives you much more control than global contrast adjustments.

Step 11: Final Adjustments and Export

Back in Lightroom (or in Photoshop), make these final checks.

Crop and straighten: Verify the horizon is level. Use the straighten tool with a reference line along the horizon if your foreground has one.

Vignette: A subtle vignette (Post-Crop Vignetting at -10 to -20 in Lightroom) draws the eye toward the center of the frame. Don't overdo it. Astrophotography already has natural falloff at the lens edges.

Check for artifacts: Zoom to 100% and scan for hot pixels (bright colored dots that aren't stars), airplane trails, or satellite streaks. Use the Spot Removal tool or Photoshop's Clone Stamp to clean these up.

Export settings: For web sharing, export as JPEG at quality 85-90, sRGB color space, long edge 2048-4096 pixels. For printing, export as 16-bit TIFF in Adobe RGB at the full resolution.

Common Mistakes to Avoid

Over-saturation. The Milky Way has real color, but it's subtle. Saturated Milky Way images with electric purples and neon blues don't look like the actual night sky. Use the Vibrance slider (+10 to +20) rather than Saturation, as Vibrance boosts muted colors without pushing already-saturated tones further.

Crushing the blacks. A completely black sky looks unnatural. There's always faint nebulosity, airglow, and light pollution gradient. Let the sky have some tone rather than forcing it to pure black.

Over-sharpening. If stars have bright halos around them, you've gone too far. Reduce the Amount and increase the Masking slider.

Ignoring the foreground. A stunning Milky Way over a murky, noisy foreground doesn't work as a cohesive image. Either light your foreground with a brief flash or headlamp during exposure, or shoot a separate longer exposure for it and blend in Photoshop.

Processing the sky and foreground identically. The sky needs different contrast, color, and noise reduction settings than the foreground. Use masks to treat them independently.

Milky Way galaxy arching over a dark landscape in Estonia
Wikimedia Commons · CC BY-SA 4.0

Recommended Software Summary

SoftwarePlatformBest ForPrice
Adobe Lightroom ClassicWindows, MacRAW processing, global edits, AI Denoise$10/month (Photography Plan)
Adobe PhotoshopWindows, MacLayer blending, masking, dodge/burnIncluded in Photography Plan
SequatorWindowsImage stacking (free)Free
Starry Landscape StackerMacImage stacking$40 (one-time)
PixInsightWindows, Mac, LinuxAdvanced astrophotography processing$230 (one-time)

For a deep dive into PixInsight, check our PixInsight beginner's guide for astrophotography.

Workflow Summary

The complete editing workflow boils down to these stages:

  1. Import and setup (profile, reset sharpening)
  2. White balance (3800-4200K, slight magenta tint)
  3. Exposure and tone (lift shadows, recover highlights, set blacks)
  4. Presence (Texture, Clarity, Dehaze for midtone punch)
  5. Tone Curve (gentle S-curve, lifted blacks)
  6. HSL/Color (warm the core, control blue saturation)
  7. Local adjustments (separate sky, core, and foreground masks)
  8. Noise reduction (AI Denoise or stacking)
  9. Sharpening (masked to stars and structure only)
  10. Photoshop (blending, curves, dodge/burn if needed)
  11. Final checks (crop, vignette, artifact removal, export)

The entire process takes 15-30 minutes once you've internalized it. The first few times will be slower as you experiment with each slider's effect. Save your settings as a Lightroom preset to use as a starting point for future images, then adjust per image as needed.

After editing, use ExifGrabber to check the original capture settings alongside your finished result. Over time, you'll build intuition for which field settings (ISO, exposure time, focal length) produce the cleanest RAW files and require the least editing to look their best.

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