Walakiri beach Stargazing & Astronomy Report
Light pollution and stargazing locations near Walakiri beach
- City
- Walakiri beach
- Country
- Indonesia
- Latitude
- -9.6286
- Longitude
- 120.4275
Key Sky Quality Metrics
- SQM (mag/arcsec²)
- 21.72
- Bortle class
- Class 2 (Class 2)
- Darkness Quotient
- 90%
- Dataset
- August 2026
Typical truly dark site
Walakiri beach: The Practical Verdict
Walakiri Beach is a remote dark site located in East Nusa Tenggara, Indonesia, boasting very dark skies. With a Bortle Class 2 rating, stargazing quality is exceptionally strong here, offering a backdrop for observing intricate cosmic details. No specific nearby destination significantly improves upon these already ideal conditions.
Under these skies, the Milky Way is clearly visible, showcasing strong structure and contrast, particularly on moonless nights. All manner of deep sky objects, including galaxies, nebulae, and meteor showers are well within reach, and broadband imaging finds strong support. While very low-altitude targets might still challenge transparency, there is no significant light pollution to contend with.
As this is already among the darker locations within the region, there is little need to seek further afield for a darker sky. Walakiri Beach is a key site for astronomy in the area.
At a Glance
- Overall
- Very strong dark sky - This is a very strong dark-sky location where the Milky Way, faint stars, nebulae, and galaxies are realistically accessible.
- Milky Way
- Clearly visible - The Milky Way should be prominent on moonless nights, with visible structure and strong contrast.
- Best targets from here
- Milky Way, galaxies, nebulae, globular clusters, open clusters, meteor showers
- Do not prioritise
- none due to light pollution alone
- Already a strong sky
- Walakiri beach is already a strong astronomy location. There is no obvious reason to travel for a darker sky.
- Long dark window
- Walakiri beach retains astronomical darkness throughout the year, so seasonality is less extreme than at higher latitudes. The main limitation is light pollution, not the length of the dark window.
Frequently Asked Questions
Can you see the Milky Way from Walakiri beach?
Yes. Walakiri beach reaches Bortle 2, dark enough that the Milky Way is clearly visible on clear, moonless nights.
What Bortle class is Walakiri beach?
Walakiri beach is Bortle Class 2 (SQM 21.72), a very strong dark sky for astronomy.
Is Walakiri beach good for stargazing?
Yes. Walakiri beach is a very strong dark sky and supports serious stargazing including deep-sky observing.
Is Walakiri beach good for astrophotography?
Broadband deep-sky imaging is realistic from Walakiri beach. Narrowband imaging of bright emission nebulae remains viable from Walakiri beach with appropriate Ha or OIII filters.
What can you observe from Walakiri beach?
Primary targets from Walakiri beach include Milky Way, galaxies, nebulae, globular clusters, open clusters. Targets such as none due to light pollution alone are not realistic from this sky.
Where are darker skies near Walakiri beach?
No meaningfully darker mapped site was found within the search radius around Walakiri beach.
When is the sky darkest in Walakiri beach?
The sky over Walakiri beach is darkest around May, June.
Is light pollution in Walakiri beach getting better or worse?
Long-term light pollution over Walakiri beach has been broadly stable across the available measurements.
north - excellent
No artificial glow on the north horizon. Faint deep-sky objects in this direction are accessible at low elevation.
north-north-east - excellent
The north-north-east horizon is fully dark. Faint stars are visible to within a few degrees of the ground and the Milky Way reaches the horizon on clear nights.
north-east - excellent
The north-east horizon is fully dark. Faint stars are visible to within a few degrees of the ground and the Milky Way reaches the horizon on clear nights.
east-north-east - excellent
Clean, fully dark horizon to the east-north-east. Star counts remain high right down to the ground.
east - excellent
The east horizon is fully dark. Faint stars are visible to within a few degrees of the ground and the Milky Way reaches the horizon on clear nights.
east-south-east - excellent
The east-south-east horizon is fully dark. Faint stars are visible to within a few degrees of the ground and the Milky Way reaches the horizon on clear nights.
south-east - excellent
Dark sky to the south-east horizon. The Milky Way can be traced to the ground in this direction.
south-south-east - excellent
Clean, fully dark horizon to the south-south-east. Star counts remain high right down to the ground.
south - excellent
The south horizon is fully dark. Faint stars are visible to within a few degrees of the ground and the Milky Way reaches the horizon on clear nights.
south-south-west - excellent
The south-south-west horizon is dark to the unaided eye. Faint stars are visible at the lowest elevations.
south-west - excellent
Clean, fully dark horizon to the south-west. Star counts remain high right down to the ground.
west-south-west - good
The west-south-west sky is dark to the horizon. Faint targets are accessible at all elevations here.
west - good
The west sky is dark to the horizon. Faint targets are accessible at all elevations here.
west-north-west - excellent
The west-north-west horizon is dark to the unaided eye. Faint stars are visible at the lowest elevations.
north-west - excellent
Dark sky to the north-west horizon. The Milky Way can be traced to the ground in this direction.
north-north-west - excellent
Dark sky to the north-north-west horizon. The Milky Way can be traced to the ground in this direction.
zenith - excellent
Dark sky overhead with a high star count. The Milky Way is visible as a structured band with cloud and lane detail.
-
Mau Ramba, East Nusa Tenggara
- Direction
- S
- Distance (km)
- 37.2
- SQM
- 21.82
- Bortle
- 2
-
Desa Waikanabu, East Nusa Tenggara
- Direction
- SW
- Distance (km)
- 45
- SQM
- 21.82
- Bortle
- 2
-
Mandahu, East Nusa Tenggara
- Direction
- WSW
- Distance (km)
- 53.4
- SQM
- 21.81
- Bortle
- 2