View of Toledo Bend on LA-TX border
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31.1965° N93.5721° WBortle 2Chicago

Toledo Bend Reservoir Photography Guide

Lake in Vernon Parish, Louisiana

  • Bortle 2 sky
  • Sunset azimuth 243°–298°
  • Clearest: October
  • Milky Way Feb–Oct
Photo: Billy Hathorn · CC BY-SA 3.0 · source

Located in Vernon Parish, Louisiana, Toledo Bend Reservoir is a lake. The nearest town is New Llano, about 30 km (19 mi) away (Toledo Bend Reservoir lies WNW of town).

Toledo Bend Reservoir is a reservoir on the Sabine River between Texas and Louisiana. The lake has an area of 185,000 acres (750 km2), the largest man-made body of water partially in both Louisiana and Texas, the largest in the South, and the fifth largest by surface acre in the United States. The dam is capable of generating 92 megawatts of electrical power. The dam itself is located in the northeast corner of Newton County, Texas; however, that county includes very little of the reservoir, as most of it extends northward into parts of Sabine and DeSoto parishes in Louisiana, and Sabine, Shelby, and Panola counties in Texas.From the Wikipedia article “Toledo Bend Reservoir”, licensed under CC BY-SA 4.0.
Nearest town
New Llano
30 km (19 mi)
Sky darkness
Bortle 2
Typical truly dark site
Clearest month
October
40% cloud
Milky Way peak
June
6.5 h window
Golden hour (Oct)
6:11 PM
sunset 6:44 PM

Light at Toledo Bend Reservoir

Live
Sunrise
7:21 AM
Sunset
6:38 PM
Golden hour AM
7:06 AM – 7:54 AM
Golden hour PM
6:05 PM – 6:53 PM
Blue hour AM
6:57 AM – 7:06 AM
Blue hour PM
6:53 PM – 7:03 PM
Full darkness
7:59 PM – 6:01 AM
Moon
Waxing Gibbous · 70%
Moonrise / set
3:29 PM / 1:49 AM
Day length
11h 17m
Sunrise azimuth
102°
Sunset azimuth
258°
000306091215182124
NightTwilightBlue hourGolden hourDaylight

Times in America/Chicago. Golden hour = sun −4° to +6°; blue hour = −6° to −4°.

Clouds at sunrise & sunset

NWS

Hourly sky cover from the National Weather Service. 20–60% cloud often gives the most colorful sunrises and sunsets.

Sunrise & sunset directions

At Toledo Bend Reservoir the sunrise point swings a long way through the year: about 62° (ENE) at the June solstice and 117° (ESE) in late December. Sunset moves from 298° (WNW) in June to 243° (WSW) in December, and the midday sun climbs to 82° in summer but only 35° in winter.

NESW60°30°
June solsticeEquinoxesDecember solstice
DateSunriseAzimuthSunsetAzimuthNoon sunDaylight
March equinox (Mar 20)7:19 AM90° E7:26 PM271° W59°12h 07m
June solstice (Jun 21)6:12 AM62° ENE8:22 PM298° WNW82°14h 11m
September equinox (Sep 22)7:03 AM89° E7:12 PM271° W59°12h 09m
December solstice (Dec 21)7:10 AM117° ESE5:17 PM243° WSW35°10h 07m

Azimuth is measured clockwise from true north (90° = east, 270° = west). Computed for 2026; values change by less than a degree from year to year.

Golden hour & blue hour by month

Lakes reflect best in calm air — usually the first hour after sunrise, before breezes ripple the surface.

Month (15th)Blue hour startsSunriseGolden hour endsGolden hour startsSunsetBlue hour endsDaylight
January6:48 AM7:14 AM7:50 AM4:59 PM5:35 PM6:01 PM10h 20m
February6:32 AM6:57 AM7:30 AM5:29 PM6:02 PM6:27 PM11h 06m
March7:01 AM7:25 AM7:57 AM6:51 PM7:23 PM7:47 PM11h 58m
April6:22 AM6:47 AM7:19 AM7:10 PM7:43 PM8:08 PM12h 56m
May5:53 AM6:19 AM6:54 AM7:29 PM8:04 PM8:30 PM13h 44m
June5:43 AM6:11 AM6:46 AM7:45 PM8:21 PM8:48 PM14h 10m
July5:54 AM6:21 AM6:56 AM7:45 PM8:20 PM8:48 PM13h 59m
August6:15 AM6:41 AM7:14 AM7:25 PM7:59 PM8:24 PM13h 18m
September6:35 AM6:59 AM7:31 AM6:50 PM7:22 PM7:46 PM12h 22m
October6:53 AM7:18 AM7:50 AM6:11 PM6:44 PM7:08 PM11h 26m
November6:17 AM6:42 AM7:17 AM4:42 PM5:17 PM5:43 PM10h 35m
December6:40 AM7:06 AM7:43 AM4:38 PM5:14 PM5:41 PM10h 08m

Local time (America/Chicago), including daylight saving time. Golden hour runs from about −4° to +6° solar altitude, so the morning golden hour begins during blue hour, before sunrise.

Milky Way & night sky

From Toledo Bend Reservoir, the Milky Way core is visible in a dark sky from February through October. June gives the longest window (about 6.5 hours on a moonless night), and the core peaks around 30° above the southern horizon. Our light-pollution model puts the sky at about Bortle 2 (typical truly dark site), which is excellent for astrophotography.

MonthCore visible (15th)HoursMax altitudeDirection
JanuaryBelow 10° in darkness—1°—
February4:43 AM – 5:33 AM0.819°SE → SE
March3:53 AM – 5:53 AM2.026°SE → SSE
April1:47 AM – 5:17 AM3.530°SE → S
May11:46 PM – 4:46 AM5.030°SE → SSW
June9:59 PM – 4:29 AM6.530°SE → SW
July9:56 PM – 3:06 AM5.230°SSE → SW
August9:26 PM – 12:56 AM3.530°S → SW
September8:43 PM – 10:53 PM2.227°SSW → SW
October8:04 PM – 9:04 PM1.019°SW → SW
NovemberBelow 10° in darkness—4°—
DecemberBelow 10° in darkness—-18°—

Window when the galactic core is at least 10° high during astronomical darkness on the 15th of each month. Pick nights within a few days of the new moon. Plan exact nights with the Milky Way planner.

Estimated sky darkness: 2 Bortle 2 — Typical truly dark site. The summer Milky Way shows rich structure; clouds look like black holes in the stars. Modeled zenith brightness ≈ 21.79 mag/arcsec².

Weather & best season

Long-term NASA satellite data for this area show October as the clearest month (about 40% average cloud cover) and February as the cloudiest (62%). August is the warmest month and January the coldest, which matters for gear, snow access and how long batteries last at night.

Average cloud cover (%)

JanFebMarAprMayJunJulAugSepOctNovDec
JanFebMarAprMayJunJulAugSepOctNovDec
High °F76818894101105107109105978880
Low °F171922334160645747352122
Precip. (in)4.44.94.94.24.14.94.14.14.14.94.35.0

Monthly climatology for the surrounding 1° grid cell from NASA POWER (MERRA-2). Mountain sites can be colder and cloudier than the cell average.

Photography tips for this lake

  • Include shoreline rocks, reeds or a log as foreground to give the reflection depth.
  • Expose for the brighter sky; reflections are typically half a stop to a stop darker.
  • After sunset, long exposures smooth wind ripples into glass.
  • For mirror reflections, get low and close to the water; the reflection grows with a lower camera.
  • A polarizer can remove reflections to show the lakebed — or keep them, depending on rotation.
  • Scout in daylight if you plan to shoot at night or before sunrise.

Season: Autumn mornings bring mist and fall color; high-elevation lakes are usually ice-free only from early summer to mid-autumn.

Suggested gear: Tripod, Circular polarizer, Wide-angle lens, Waterproof boots. Work out exposures with the depth of field, ND filter and NPF rule calculators.

Nearby photo spots

Other locations within 25 km of Toledo Bend Reservoir, closest first.

FAQ

When is the best time to photograph Toledo Bend Reservoir?
October has the clearest skies on average; june is best for the milky way core. For light, plan around the first and last hour of sun. Autumn mornings bring mist and fall color; high-elevation lakes are usually ice-free only from early summer to mid-autumn.
What time is golden hour at Toledo Bend Reservoir?
In October the evening golden hour starts around 6:11 PM and ends after sunset at about 6:44 PM; the morning golden hour lasts until about 7:50 AM. Use the live widget above for exact times on any date.
Where does the sun rise and set at Toledo Bend Reservoir?
Sunrise azimuth ranges from about 62° in June to 117° in December; sunset ranges from 298° to 243°. See the sun-path diagram for the full arc.
Can you see the Milky Way from Toledo Bend Reservoir?
Yes — the core is visible from February to October on moonless nights. The estimated sky quality is Bortle 2 (typical truly dark site).
Do you need a permit to photograph at Toledo Bend Reservoir?
Personal photography from public land rarely needs a permit. Commercial shoots, models, large groups and drones may require permission from the land manager — check before you go.
How far is Toledo Bend Reservoir from New Llano?
About 30 km (19 mi) in a straight line; driving distance is usually longer, especially in mountain terrain.

Sources

Location data: Wikidata, Wikipedia. Sun, moon and Milky Way times are computed by LWPhoto Atlas for 2026. Climate: NASA POWER. Sky darkness is a population-based estimate (Walker's law), not a measurement. See data sources & licenses.