AstronomyHow To

How to Photograph the Milky Way With Your Smartphone: No Gear, No Experience, No Excuses

Muhammad Jawad Published August 1, 2026 · 11 Min Read

Last updated: August 14, 2026

Contents
  1. What You'll Need
  2. How Smartphones Capture the Milky Way
  3. Best Time of Year to Photograph the Milky Way
  4. How to Stabilize Your Phone for Astrophotography: No Tripod Needed
  5. Best Camera Settings for Milky Way Photography with Smartphone
  6. iPhone
  7. Android
  8. How to Find and Frame the Galactic Core
  9. Editing Milky Way Photos on Your Phone
  10. Quick Troubleshooting
  11. One Last Thing
  12. Frequently Asked Question
  13. Can any smartphone photograph the Milky Way?+
  14. Do I need a tripod to photograph the Milky Way?+
  15. What's the best ISO for Milky Way photography on a smartphone?+
  16. Why can't I see the Milky Way even though the app says it's there?+
  17. Can I photograph the Milky Way in winter?+

Before you head out, make sure you have:

  • Smartphone with Night Mode or Manual/Pro Mode
  • Dark sky (Bortle Class 4 or darker)
  • Stable support or tripod
  • Clear, moonless night
  • Fully charged battery
  • Patience
Comparison showing how the Milky Way appears to the human eye versus a smartphone long-exposure photograph.
The human eye sees a faint, silvery band, while long-exposure smartphone photography reveals far more detail and color.
A smartphone stabilized in a hiking boot for long-exposure Milky Way photography without a tripod.
A sturdy hiking boot can serve as a surprisingly stable support when you don’t have a tripod.
Smartphone mounted on a tripod using manual camera settings for Milky Way photography.
A stable tripod and manual camera settings greatly improve your chances of capturing a sharp Milky Way image.
Using a smartphone app to plan Milky Way photography before photographing the galaxy
Astronomy apps help you locate the Milky Way’s galactic core before you begin shooting.
Milky Way photography with smartphone at a mountain campsite under a dark sky
Finding a truly dark sky matters more than owning an expensive camera.

Written by

Muhammad Jawad

Muhammad Jawad writes Earthshine Journal's stargazing, dark-sky travel and camping coverage. Published work includes beginner guides to the night sky, smartphone astrophotography, dark-sky destination research, camp cooking and night-time safety outdoors, alongside science explainers on subjects such as wind and Saturn's ring plane crossing. Articles published under this byline are researched and fact-checked in line with the Editorial Policy.

Up Next
Scientific visualization of what happens when black holes collide, showing two dark event horizons bending background starlight just before merging.
AstronomyScience

What Happens When Two Black Holes Collide?

Two black holes in orbit around each other lose energy, spiral inward, and eventually merge into a single larger black hole. That much is simple. What happens when black holes collide gets strange in the accounting.On 14 September 2015, detectors in Louisiana and Washington State recorded the final moments of two black holes of roughly 36 and 29 solar masses. The black hole they became weighed about 62 solar masses, not 65. The missing three solar masses did not go anywhere in the ordinary sense. It was converted into gravitational waves and radiated away as ripples in the shape of spacetime itself.For a fraction of a second, the power flowing out of that collision was more than ten times the combined light output of every star in every galaxy in the observable universe. It produced no light at all.When black holes collide, what is actually colliding?Two black holes do not collide in the way two rocks do, because there is nothing solid to make contact.A black hole is a region where gravity is strong enough that nothing, including light, can escape. Its boundary is the event horizon, which is not a surface but a location: the point beyond which every possible path leads inward. There is no material there to crash.When two of them orbit closely, general relativity says the orbit itself radiates energy as gravitational waves. Losing energy means the orbit tightens, which makes them orbit faster, which radiates energy faster. The process runs away. Over millions of years the inspiral is imperceptible, and in the final second the two objects sweep around each other dozens of times before their horizons merge into one.What emerges is a single black hole that briefly wobbles, like a struck bell, before settling into a smooth stable shape. That final wobble is called the ringdown, and it is visible in the data.Three Suns' worth of mass became pure spacetime rippleThe energy released is the part worth slowing down for, because it is hard to place on any familiar scale.In the 2015 event, catalogued as GW150914, about 3.0 solar masses were radiated as gravitational waves, roughly 5.4 × 10^47 joules. That is mass converted directly into energy, the relationship Einstein wrote down in 1905, applied at a scale nothing else in the universe reaches.The peak power matters more than the total. LIGO's estimate is that in the final moments the collision radiated more than ten times the power of all the light from all the stars and galaxies in the observable universe,…

Continue Reading