Great Sand Dunes National Park and Preserve
One-line summary: The tallest dunes in North America (Star Dune ~750 ft; Hidden Dune ~741 ft) piled in the San Luis Valley by a wind regime that traps sand between southwesterly prevailing winds off ancient lakebeds and opposing northeasterly winds spilling back over the Sangre de Cristos — plus seasonal Medano Creek, whose globally rare "surge flow" pulses waves of water along the dune base in late spring, and an International Dark Sky Park surrounded by 14ers.
Great Sand Dunes National Park and Preserve
One-line summary: The tallest dunes in North America (Star Dune ~750 ft; Hidden Dune ~741 ft) piled in the San Luis Valley by a wind regime that traps sand between southwesterly prevailing winds off ancient lakebeds and opposing northeasterly winds spilling back over the Sangre de Cristos — plus seasonal Medano Creek, whose globally rare "surge flow" pulses waves of water along the dune base in late spring, and an International Dark Sky Park surrounded by 14ers.
Scope note: this template covers steps 1–3 of the adventures pipeline (identify, support Maxine's research, shape goals). The deliverable webpage
- video at step 6 is Maxine's own work — don't scaffold it here.
Links & Maps
Official:
- Site: https://www.nps.gov/grsa/index.htm
- Fees: https://www.nps.gov/grsa/planyourvisit/fees.htm
- Hours / VC: https://www.nps.gov/grsa/planyourvisit/hours.htm
- Camping: https://www.nps.gov/grsa/planyourvisit/camping.htm
- Recreation.gov (campsite reservations): https://www.recreation.gov/camping/campgrounds/234072
- Medano Creek surge flow status (live): https://www.nps.gov/grsa/learn/nature/medanocreek.htm
- Astronomy / dark sky: https://www.nps.gov/grsa/planyourvisit/nightskyprograms.htm
Maps:
- Google Maps (Visitor Center): https://www.google.com/maps/place/Great+Sand+Dunes+National+Park+%26+Preserve
- NPS map: https://www.nps.gov/grsa/planyourvisit/maps.htm
- USGS topo: search "USGS Liberty CO 7.5 quad" (covers dunefield)
Reference & background:
- Wikipedia, Great Sand Dunes NP: https://en.wikipedia.org/wiki/Great_Sand_Dunes_National_Park_and_Preserve
- NPS Geodiversity Atlas — Great Sand Dunes: https://www.nps.gov/articles/nps-geodiversity-atlas-great-sand-dunes-national-park-and-preserve.htm
- Madole et al., "Origin of the Great Sand Dunes" (USGS Professional Paper, search USGS for the open-file) — the canonical source on dunefield formation
- Surge flow in Medano Creek (peer-reviewed): search "Schumm and Khan antidune surge flow Medano"
- International Dark-Sky Association (Great Sand Dunes is a Gold Tier IDSP): https://darksky.org/
- Wikipedia, Aeolian processes (dune physics primer): https://en.wikipedia.org/wiki/Aeolian_processes
Site geography (read before planning the day)
Great Sand Dunes is not a typical desert dunefield — it's a 30-square-mile sand pile built and trapped in a specific spot by a peculiar wind regime. The components:
- Source sediment: the San Luis Valley is an ancient intermontane basin between the San Juan Mountains (west) and the Sangre de Cristos (east). The valley floor holds vast lakebed and alluvial sediments — the "San Luis Lake" of the Pleistocene drained ~440,000 years ago through what's now the Rio Grande, leaving behind the valley sediments that are the dune source.
- Sand transport: prevailing southwesterly winds sweep sand from the valley floor northeast across the basin.
- The trap: the sand piles up against the Sangre de Cristo Range, but doesn't go over — because the mountains channel opposing northeasterly winds down through three passes (Medano, Music, and Mosca Passes). The opposing wind pushes the leading dune face back. The result is a remarkably stable dunefield that pulses but doesn't migrate over geological time.
- The water seal: Medano Creek (from the east, fed by Sangre de Cristo snowmelt) and the seasonal water table mark the southeastern dunefield boundary, with the creek literally pulsing in May–June via the surge flow mechanism.
The big dunes — Star Dune (~755 ft, possibly the tallest in North America when measured base-to-crest), Hidden Dune (~741 ft, very close), and High Dune (~699 ft, the more commonly hiked "summit" with the easier access) — are all visible from the main parking lot. The dunefield is bordered on the east by the Sangre de Cristo Wilderness (the "Preserve" part of the park's name) with several 13,000 and 14,000 ft peaks within visual range — Mount Herard (13,345), Cleveland Peak (13,414), Crestone Peak (14,300 ft, 7th-highest in CO).
Critical: the main parking lot is at 8,175 ft, the base of the dunes is at ~8,200 ft, and High Dune is at ~8,895 ft. Star Dune is about ~8,950 ft. So the dune-top altitude is real but not Mt-Blue-Sky scary. The killer at the dunes is not altitude — it's heat, wind, and sun.
Must-See / Big Items
Ranked by payoff. Order assumes 2–3 days on site.
- Walking onto the dunes from the main parking lot — there's no trail. You walk across Medano Creek (May–June), then start up the sand. This is the central park experience. Go at dawn or dusk; midday in summer the sand is genuinely scalding.
- High Dune (~699 ft above base, 2.5 mi RT but it's sand) — the standard dune "summit" hike. Not technically the tallest, but accessible. Takes 2–3 hours up + 30 min down (descending sand is fast). From the top: 360° view of Sangre de Cristos, dunefield geometry, San Luis Valley. The hardest 700 ft of elevation gain you'll ever do — sand absorbs every step.
- Star Dune (the actual tallest, ~755 ft, 8 mi RT) — much harder; requires committing to a full half-day on the sand. The route traverses the dunefield. Few people do it. Worth it as a challenge for a strong 12-year-old in good weather. Don't try in summer.
- Medano Creek + surge flow (mid-May to early June only) — the seasonal creek peaks late May. The "surge flow" phenomenon: the creek pulses in waves, roughly 30 seconds apart, caused by sandbed-instability dynamics (antidunes building, breaking, re-building). Found in only a handful of places globally. Wade, splash, sit in it, watch the surges build and break. The "beach" along the creek is one of the trip-prize photo settings.
- Sand-sledding / sandboarding — boards rent in Alamosa (Kristi Mountain Sports) or just outside the park (Oasis Store). Regular sleds don't work; you need a waxed sandboard. Climb a steep dune face, sit or stand, slide down. Maxine should LOVE this. Pre-9am or post-5pm in summer to avoid burning sand.
- Sunset on the dunes — the light raking the dune faces at sunset creates shadow geometry that the camera can't quite capture but the eye locks onto. From the main parking lot lookout or, better, from a position 1/4 mi out on the dunefield itself.
- Night sky / star party — Gold Tier International Dark Sky Park. The Milky Way over the dunes with the Sangre de Cristos as a silhouette is one of the great American astronomy views. NPS hosts free ranger-led night-sky programs in summer; check schedule. Bring binoculars at minimum.
- Mosca Pass Trail (7 mi RT, 1,400 ft gain, moderate) — a hike up into the Sangre de Cristos, away from the dunes. Good complement: walk up through aspen and conifers, look back at the dunefield from above. Mosca Pass itself was a historical wagon route.
- Medano Pass 4WD Road (22 mi one-way, requires 4WD + low-clearance is dangerous) — for the rental car this is usually out, but worth knowing about. Fords Medano Creek several times. Connects park to the Wet Mountain Valley. If you have the right vehicle, it's a 4-hour adventure.
- Zapata Falls — outside the park (~12 mi south), USFS land. Short hike (0.5 mi) to a falls hidden in a slot canyon. Easy and very different from the dunes; good shoulder activity. Best in spring snowmelt.
Stretch goals (do if time allows):
- San Luis Lakes State Wildlife Area — 30 min away, wetland birding (sandhill cranes Feb–Mar and Sep–Oct; the entire crane migration funnels through the San Luis Valley).
- Crestone, CO — 30 min N, eccentric spiritual-retreat town at the base of the 14ers. Great breakfast spot (Cloud Station).
- UFO Watchtower (Hooper, CO) — kitschy private roadside attraction north of the park; Maxine might find it charming/funny.
- Alamosa NWR + Monte Vista NWR — refuge complex south/west of Alamosa, more crane and waterfowl habitat.
- Sand Creek Massacre NHS — ~3 hr east. If the Colorado trip is also doing Mount Blue Sky, this is the third leg of an Indigenous-history thread.
Research angles for Maxine
The research is hers — list questions to investigate and sources to start from, not answers. Pitch above grade level.
Hook into Maxine's current interests: (ask before finalizing — what is she into right now? If she's currently on a physics kick, push the aeolian-process + surge-flow physics threads. If it's geology, push the basin-and-range + dunefield-stability threads. If it's astronomy, push the dark-sky thread. If it's biology, push the kangaroo-rat + Tiger Beetle endemism. If it's writing, push the place-portrait of a non-iconic landscape.)
Questions worth chasing:
- Science (aeolian processes): Sand moves in three modes — suspension (small grains, lifted high), saltation (most of the mass, bouncing along the surface), creep (largest grains, rolling). What's the wind velocity threshold for each at the GSDNP grain size (mostly 0.2–0.5 mm)? What are the slip face geometry (the steeper, leeward side, at the angle of repose ~33–34°) and stoss face (the gentler windward side)? Why does a dune migrate, and why don't the Great Sand Dunes migrate (much)?
- Science (dunefield stability): Most dunefields are migratory — they move downwind over decades to millennia. GSDNP is famously stable — the dunes pulse and reform locally but the dunefield boundary hasn't moved much in ~10,000 years. Why? (Hint: opposing-wind regimes through Medano, Music, and Mosca passes counter the prevailing SW winds.) Map the wind-rose and dune-orientation relationship. Compare to a migratory dunefield like White Sands (NM) or Algodones (CA).
- Science (sand provenance): Where did the sand come from? It's not desert weathering — it's lakebed and alluvial sediments from the Pleistocene Lake Alamosa that filled the San Luis Valley until ~440,000 years ago. Mineralogically, the sand is mostly quartz with feldspar and some volcanic glass — the volcanic glass fingerprints the San Juan Mountains to the west as a source. How do you do provenance analysis on a sand grain?
- Science (surge flow / antidunes): Medano Creek's "surge flow" is a globally rare phenomenon — the creek pulses water in waves, roughly 20–30 seconds apart. Why? It's a hydraulic jump cycle on a mobile sandbed: small antidunes form on the bed, build up, break (release water and sand downstream), then reform. The Froude number > 1 (supercritical flow) is necessary. Where else on Earth does this happen? (Only a handful: Mosi-oa-Tunya rapids at Victoria Falls in some seasons, parts of the South Platte, the Río Coyle in Argentina, sections of the Indus.)
- Science (dunefield ecology): Two endemic species live nowhere else: the Great Sand Dunes Tiger Beetle (Cicindela theatina, the official park beetle) and the giant sand-treader camel cricket (Daihinibaenetes giganteus). Plus the Ord's kangaroo rat (Dipodomys ordii) is the dominant nocturnal mammal. How do these animals handle 150°F surface sand and zero water? (Burrowing for daytime hiding, nocturnal activity, metabolic water from food, kidney concentration for the kangaroo rat.) The plains pocket mouse also burrows.
- Science (dark sky): GSDNP is a Gold Tier International Dark Sky Park — the highest IDA designation. Bortle Class 2 (excellent dark sky) at the dunefield. What does the Milky Way look like at Bortle 2 vs. Bortle 6 (Austin)? Compare to other dark-sky sites she's been to (Big Bend NP, McDonald Observatory). How is "dark sky" measured — sky-quality meter (SQM) readings, Bortle subjective scale, satellite light-pollution maps?
- Science (geomorphology): The whole Great Sand Dunes system is fed and bounded by a closed hydrology. Sand-laden winds carry sand in; Medano Creek carries some sand out (eastward, redepositing it on the sand sheet); the sand sheet (the apron of low dunes south and west of the main field) is the "feeder" reservoir. This is a self-regulating system. Map the sand budget — in vs. out — using the NPS's own published estimates.
- Science (Pleistocene context): The dunefield is mostly built since ~12,000 years ago, after the last glacial maximum. Before that, glaciers in the Sangre de Cristos carried different sediment loads, and Lake Alamosa in the valley was much larger. What was this landscape like 20,000 years ago vs. 12,000 years ago vs. now? How does the dune chronology tie to climate change since the Younger Dryas?
- History (Indigenous): The dunes are sacred to the Diné (Navajo), Pueblo, Ute, and Jicarilla Apache peoples — present in oral tradition as a site of creation stories, sometimes called Sei-anyedi in Apache or referenced in Navajo emergence stories. What's the cultural-property status of the dunefield, and how does the park work with affiliated tribes today? (Search NPS's Tribal Consultation pages.)
- History (Pike + Frémont): Zebulon Pike crossed the San Luis Valley in 1807 (and was promptly captured by Spanish authorities — the U.S.-Mexico border was just south of here). John C. Frémont's 1848 expedition disaster (his Fourth Expedition lost 10 men in the winter Sangres). What were these explorers actually looking for, and what did they get wrong?
- History (park designation): Designated a National Monument in 1932 (Herbert Hoover signed). Redesignated National Park and Preserve in 2004 (this added the surrounding wilderness lands — Preserve allows hunting; Park doesn't). What was the campaign to upgrade NM → NP&P, and what does the distinction do legally?
- Writing: Spend an hour walking out into the dunefield with no headphones, no camera (or camera off). Then write a 600-word place-portrait. Constraint: don't describe what the dunes look like (no comparison to ocean waves, no comparison to deserts, etc.). Describe what they are — texture, sound, the way the wind sounds at 200 ft up the slip face.
- Writing (process): Write a technical description of how a single sand grain travels from the San Juan Mountains to High Dune. Cover ~10 million years, multiple modes (river, lake, wind), and ~150 miles. Use the actual mineralogy.
- Math (saltation): For typical GSDNP sand (median grain diameter ~0.3 mm, density ~2,650 kg/m³) and 20 m/s wind, compute the saltation hop length using Bagnold's classic equation (~10–15 grain diameters per hop average). How many hops does a grain make to cross 1 mile?
- Math (dune migration in a steady wind): Even though GSDNP doesn't migrate at the dunefield scale, individual dune crests do shift seasonally. If a 200-ft dune migrates at 1 m/year under a one-sided wind, how long would it take to traverse 30 miles? Compare to the actual ~10,000-year dunefield age.
- Math (surge flow Froude number): Estimate Medano Creek's velocity (timed float of a stick over a known distance), depth (a meter stick), and width during peak surge. Compute Froude number F = v / √(g × d). Is F > 1 (supercritical)? What's the wave celerity vs. flow velocity?
- Math (heat): Sand at noon in July reaches 140–150°F. Air temperature might be 80°F. Why the difference? Compute the energy balance: incoming solar radiation, albedo of sand (~0.4), thermal conductivity vs. heat capacity. Why does the surface heat so much faster than the air? Why is the sand 10 cm down much cooler than the surface?
- Math (dark sky): Sky brightness at GSDNP measured in SQM ~21.8 mag/arcsec². Austin sky might be ~18.5. That's a difference of 3.3 magnitudes = a factor of ~21× brightness difference. So an Austin observer sees the sky as ~21× brighter than at GSDNP. Compute the implied difference in faintest visible star (use the formula: each magnitude is a factor of ~2.512).
- Art (light + texture): Photography of dunes is famously about texture and shadow, not color. Build a portfolio: same dune face at sunrise, noon, sunset. Same dune at low-angle vs. high-angle light. Black-and-white treatment vs. color. Compare to the Edward Weston / Brett Weston dune photographs (Death Valley and Oceano, CA).
- Art (sound): "Singing sands" — some dunes globally produce audible sound when sand cascades down a slip face (it's a stick-slip vibration of layered grains). GSDNP does this sometimes. Set up a phone recorder, slide down a steep slip face, record the sound. Compare to recordings of the Algodones Dunes or Mongolian "booming" dunes.
Starting sources (not exhaustive — she'll find more):
- NPS GSDNP "Learn" portal: https://www.nps.gov/grsa/learn/index.htm
- Madole et al. USGS papers on dunefield formation
- Bagnold, R.A. (1941). The Physics of Blown Sand and Desert Dunes — the founding text on aeolian science. Some sections are dense but the diagrams are timeless.
- Schumm & Khan on antidune surge flow (peer-reviewed journals — search "Medano Creek antidunes")
- "Roadside Geology of Colorado" — relevant chapter
- NPS soundscape recordings of "singing sands": https://www.nps.gov/subjects/sound/
- International Dark-Sky Association GSDNP designation: https://darksky.org/places/great-sand-dunes-national-park-and-preserve/
- Wallace Stegner, Beyond the Hundredth Meridian — context for John Wesley Powell-era exploration of the West that included this region
- Jicarilla Apache oral histories — start with Morris Edward Opler's 1938 ethnographies (peer-reviewed sources)
Observable field goals
Goals Maxine can verify or document in the field at step 5 (confirm & document). Concrete things to look at, count, measure, identify, or photograph — not vague "learn about X."
- Walk to the top of High Dune. Photograph: (a) the dunefield panorama, (b) the Sangre de Cristos to the east, (c) the San Luis Valley to the west. Record altitude, time, temperature, wind speed.
- On a dune slip face: identify the angle of repose by direct measurement (use a phone inclinometer). Confirm it's ~33–34°. Note which side is the slip face and which is the stoss face. Photograph the lee-side wind-rippled surface vs. the smooth slip face.
- If May–June: at Medano Creek, time the surge cycle. Use a stopwatch — count seconds between visible wave fronts. Take a video showing at least 3 surge cycles. Estimate the wave height. Note the creek's width, depth (use a stick), and approximate flow velocity (time a leaf floating over a known distance).
- Photograph at least one sand-ripple pattern. Note the wavelength (crest-to-crest distance) and orientation relative to the current wind direction. Sand ripples form perpendicular to the wind.
- Find tracks in the sand. Identify and photograph at least 3 different track types — likely candidates: kangaroo rat, beetle, lizard, raven, coyote. (Best at dawn before crowds + wind erase them.) Bonus: photograph a live Great Sand Dunes Tiger Beetle (Cicindela theatina) — they're active in summer, often near the creek.
- Record sand temperature at three times: mid-morning, noon, late afternoon. Use a phone thermometer or buried thermometer. Bury a thermometer 10 cm down — compare to surface temp.
- Night sky: photograph the Milky Way over the dunes (long-exposure phone shot or DSLR). Estimate magnitude limit by counting visible stars in a known constellation (e.g., Little Dipper — at Bortle 2, all 7 stars including the 5.0-mag Polaris-region stars should be naked-eye).
- Sand sample: take a small (1 tsp) jar of dune sand home. Outside the park boundary — sand collection is not allowed inside the NP. The sand sheet south of the park (USFS or BLM land) allows it. Examine under hand lens at home; identify quartz vs. feldspar vs. dark volcanic grains.
- If sand-sledding: time her descent. Compute average speed. Note how friction (waxed vs. unwaxed board) affects it.
- At sunset: photograph the same dune from the same spot every 15 minutes for an hour as the light angle changes. Note how shadow geometry transforms the same physical shape.
- Wildlife / bird log: ID at least 5 species over the trip. Likely: common raven, magpie, mountain bluebird, mule deer, pronghorn (in the valley), kangaroo rat tracks, possibly elk in the preserve. In spring, sandhill cranes passing through the valley.
Suggested itinerary
3-day plan, base in Alamosa or Piñon Flats Campground in-park.
Day 1 — Drive in from Denver area or COS, gentle afternoon
- Arrive in Alamosa by mid-afternoon. Check in to lodging. Stock up on water, snacks, sunscreen, sand-board rental.
- 4:00 pm drive to GSDNP (~35 min from Alamosa). Visitor Center orientation. Watch the introductory film. Talk to rangers about Medano Creek current status (if May–June) and any ranger programs that night.
- 5:00 pm — first walk onto the dunes. Don't hike up High Dune today — just get on the sand, splash in Medano Creek (May–June), feel the scale. ~1 hour out and back.
- Sunset on the dunes — most people walk back at sunset. Position yourself 1/4 mi out on the dunefield itself looking back at the Sangre de Cristos with light raking across the dunes.
- Dinner at the lodge or in Alamosa.
- Night sky observation — if no ranger program, head back to the dunes parking lot after dinner. Pulses of headlights on the dunes will be other dark-sky chasers; that's expected. Find your own quiet patch.
Day 2 — Big dune day
- 5:30 am alarm. Pre-dawn drive to the main parking lot. Sunrise on the dunes — light just barely catching the eastern faces. Photographs.
- 6:30 am — start the High Dune (or Star Dune if she's strong + acclimatized) hike. Carry 1 gal water per person, snacks, sunscreen, wind layer.
- 9:30–10:30 am — back at the parking lot. The day's serious dune time is now over (sand temps rising).
- 11:00 am — Medano Creek wade + surge-flow observation (if May–June). Time the surge cycles. Sand-sled the dune face near the creek.
- 12:30 pm — drive to Alamosa for AC lunch. Long break in the heat.
- 3:00 pm — Zapata Falls (~12 mi S, short hike to slot-canyon falls — different scenery).
- 5:30 pm — back to the dunes for late-afternoon light. Optional sandboarding session.
- Night — second night of star observation. NPS may run a ranger program. Look for Andromeda, the Milky Way core (in summer), and any meteor shower active (Perseids in August, etc.).
Day 3 — Side hike + drive out
- 7:00 am — Mosca Pass Trail (7 mi RT, 1,400 ft). A into-the-mountains hike for contrast: aspen, conifer, alpine views back at the dunefield. ~4 hours.
- 11:30 am — pack up. Drive home or continue to Pikes Peak / Cripple Creek / Colorado Springs for the trip's next leg.
Family roles:
- Chris leads: logistics, water management (this is genuinely dangerous in summer heat — overhydrate), driving the long approach. Sets the dune-hike turnaround time.
- Heather leads: the early-morning photography and wildlife eye, the Medano Creek surge-flow timing, the sand-sledding fun (she'll be better at it than Chris).
- Maxine drives: the surge-flow physics experiment (Froude number from her own measurements), the sand-sample collection + ID, the dark-sky observation log. Picks the dominant lens — physics (surge flow + saltation math), geology (provenance + dunefield stability), astronomy (Bortle 2 sky), or wilderness ecology (Tiger Beetle + kangaroo rat).
- Solo vs. both parents: both. Heat + sand + remote location = real safety stakes; don't split the family far on the dunes.
Connections
Combines well with:
- Pikes Peak — 2.5 hr north. Same Sangre de Cristo / Front Range basement geology, dramatically different exposure. Logical 4–5 day Colorado Springs + GSDNP trip.
- Cripple Creek — 2 hr N, gold-mining town on the way to/from Pikes Peak.
- Royal Gorge — 2 hr N. Logical stop on the way back to Denver.
- Florissant Fossil Beds — between GSDNP and Colorado Springs. Eocene paleobotany contrasts beautifully with the modern aeolian geology here.
- Big Bend National Park — Chihuahuan Desert comparison, especially for dark-sky and aeolian-process content. Different geology (volcanic vs. sand piling) but kindred remote/dark-sky character.
- McDonald Observatory — both are Gold-Tier dark-sky sites. A "dark sky western tour" project could link McDonald, Big Bend, and GSDNP.
Feeds into home projects / future adventures:
- An aeolian-physics unit (saltation, dune migration, dunefield stability) using GSDNP measurements.
- A surge-flow / hydraulics project — Froude number, antidunes, supercritical flow. Hard physics, fun field experiment.
- A "tallest dunefields on Earth" comparative project: GSDNP (~755 ft), Cerro Blanco in Peru (~3,860 ft, world's tallest), Badain Jaran in China (~1,640 ft), Erg Chebbi in Morocco. Why are some bigger?
- A dark-sky observation log continuing from Big Bend / McDonald.
- Future trip: White Sands NP (NM) — gypsum dunes, very different mineralogy, ~4 hr from GSDNP. Logical sequel.
- Future trip: Death Valley NP (CA) — different desert physics, lower altitude, broader temperature range.
Open questions / still to research (Chris's side)
- Lock the trip window. Late May / early June is the Medano Creek prize window but also competing with high tourism. Late September (no creek but cool temps + dark October moon) is a fallback.
- Book Piñon Flats Campground 6 months ahead if camping; otherwise lock Alamosa lodging.
- Verify current Medano Creek peak flow date (the NPS Medano Creek page publishes a real-time update each spring).
- Rent sandboards — Kristi Mountain Sports in Alamosa or the Oasis Store right outside the park. Confirm hours.
- Pre-trip reading list: NPS surge-flow page, one aeolian-physics primer, dunefield stability paper.
- Decide combine plan: GSDNP-only vs. GSDNP + Pikes Peak + Cripple Creek + Florissant (5+ day loop) vs. GSDNP + Sand Creek Massacre NHS (Indigenous-history thread).
- Verify night-sky / ranger program schedule for the trip dates.
- Get a Bortle scale primer + SQM reading from home in Austin for baseline comparison.
- Confirm flight option — direct AUS → COS may be more efficient than AUS → DEN for this trip.
- Sun + heat plan: hat selection, electrolyte mix (just water isn't enough at altitude in heat), backup retreat plan if temps exceed 95°F.
- Decide whether to add the Medano Pass 4WD road — requires a real 4WD rental, an extra adventure but not for a standard rental car.
- Pre-trip: review aeolian physics basics with Maxine so the field measurements have a framework — at minimum the saltation/suspension/creep distinction and the angle-of-repose concept.