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View of Priest Rapids Bar

The Priest Rapids Bar is one of the most massive Ice Age Floods gravel bars in existence -- a mountain of flood debris rising over 400 feet above the Columbia River and covering an enormous area south of the Saddle Mountains. To put its scale in perspective, this single gravel...

Location
46.6389°, -119.7320°WGS84
Trail
Ice Age Floods NGTWA / OR / ID / MT
Type
Geological sitePOI

The Priest Rapids Bar is one of the most massive Ice Age Floods gravel bars in existence -- a mountain of flood debris rising over 400 feet above the Columbia River and covering an enormous area south of the Saddle Mountains. To put its scale in perspective, this single gravel bar is taller than a 40-story building and contains enough material to bury a small city. The bar was deposited when floodwaters decelerated after passing through gaps in the Saddle Mountains, dropping their massive sediment load of boulders, cobbles, and gravel in a sprawling fan-shaped deposit. The size of the boulders within the bar -- some weighing many tons -- indicates the extraordinary velocity and carrying capacity of the floodwaters that transported them. The bar is best viewed from the pullout along the highway, where its sheer scale becomes apparent against the backdrop of the Columbia River below. Gravel bars of this magnitude are found nowhere else on Earth outside the Ice Age Floods region, and the Priest Rapids Bar is among the largest of them all. It is perhaps the single most impressive piece of evidence for the floods' raw sediment-moving power.

Site research

Status & accessibility

The bar itself is on Wahluke Slope (east bank of the Columbia between Vernita Bridge and Sentinel Gap) and is largely on the Hanford Reach National Monument; vehicular access is limited. The best public viewpoints are pullouts on State Route 24 descending from the Wahluke Slope, and from the Vernita Bridge area on SR 24 / SR 243. No fees; daylight hours only on monument land.

Ice Age Floods context

Priest Rapids Bar (also called Wahluke Bar or Mattawa Bar) is one of the largest expansion bars left by the Missoula floods. As flood pulses surged south through Sentinel Gap and Frenchman Hills, the flow expanded into the Pasco Basin and dropped its bedload. The bar surface stands roughly 430 ft above the modern Columbia, and the gravel package contains boulders up to ~1.4 m in diameter. Bar elevation and stratigraphy mark the lower bound on flood depth through this reach (Lake Lewis was deeper still upstream behind Wallula Gap). The bar surface also carries flood-current bedforms visible on lidar.

Recent research

No Priest Rapids Bar–specific dating studies have been published since the Balbas et al. (2017) chronology, which dates the largest flood through this reach at 18.2 ± 1.5 ka.

IAFI presence

The IAFI Lake Lewis Chapter covers this stretch in its Lake Lewis Floodscape brochure. No on-site IAFI signage at the bar itself.

Visitor info

Best in late spring or fall when haze is low. The Wahluke Slope pullouts give a long view down-bar; combine with the Wanapum Vista pullout to the north and the White Bluffs Overlook to the south for a half-day Lake Lewis geology loop.

Sources

  • https://washingtonlandscape.blogspot.com/2013/12/notes-on-richland-to-sentinel-gap-fog.html
  • http://iceagefloods.blogspot.com/2009/10/sentinel-gap-and-mattawa-bar.html
  • https://wa100.dnr.wa.gov/columbia-basin/ice-age-floods
Capture roadmap

What this site looks like once Phase 1 lands.

Every site along the trail will receive the full Terrain360 capture treatment: ground-level 360° panoramas, drone aerial imagery, and photogrammetry-based 3D models that visitors can spin in their browser. This page reserves the slots; the imagery flows in as field capture completes.

360° panoramic

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Phase 1 target · June–July 2026
Drone aerial

Read the landscape from above

Drone flyovers reveal the geometry of catastrophe — ripple marks, gravel bars, and scour patterns invisible from the ground.

Phase 1 target · June–July 2026
3D photogrammetry

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Photogrammetry and Gaussian-splat models let visitors rotate, measure, and inspect features in detail-page WebGL viewers.

Phase 1 target · June–July 2026