Top Tweets for #rosettacliffs

about 1 year ago

🟥 ⛏️ Hathor region of comet 67P Churyumov–Gerasimenko's larger lobe, revealing a cliff face that towers approximately 1 km high, formed from layered, consolidated material of ice, dust, and organics. ❤️ 🔁 #Comet67P #RosettaCliffs 🎞 @TrendingFutureTimes ▶️ The cliff exhibits prominent fractures, overhangs, and irregular outcrops, indicative of mechanical erosion, gravitational slumping, and sublimation-driven retreat as volatiles escape into space. The base transitions to a smoother talus-like slope blanketed in fine-grained regolith and scattered meter-scale boulders, representing debris from episodic cliff collapses and dust deposition. Overall, the terrain reflects the comet's low-density, porous structure (around 0.5–0.6 g/cm³), with subdued craters due to ongoing resurfacing processes.

$geologyBits's tweet photo. 🟥 ⛏️ Hathor region of comet 67P Churyumov–Gerasimenko's larger lobe, revealing a cliff face that towers approximately 1 km high, formed from layered, consolidated material of ice, dust, and organics. ❤️ 🔁 #Comet67P #RosettaCliffs 🎞 @TrendingFutureTimes ▶️ The cliff exhibits prominent fractures, overhangs, and irregular outcrops, indicative of mechanical erosion, gravitational slumping, and sublimation-driven retreat as volatiles escape into space. The base transitions to a smoother talus-like slope blanketed in fine-grained regolith and scattered meter-scale boulders, representing debris from episodic cliff collapses and dust deposition. Overall, the terrain reflects the comet's low-density, porous structure (around 0.5–0.6 g/cm³), with subdued craters due to ongoing resurfacing processes.$

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