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A grayscale image from the Dawn spacecraft showing Occator Crater on Ceres, the largest object in the asteroid belt.  Bright spots within the crater remain a mystery despite high-resolution images.  A faint haze is also visible above the crater.  The image is a composite from recent observations.

A grayscale image from the Dawn spacecraft showing Occator Crater on Ceres, the largest object in the asteroid belt. Bright spots within the crater remain a mystery despite high-resolution images. A faint haze is also visible above the crater. The image is a composite from recent observations.

Astronomy Picture from 16/09/2015

Bright Spots Resolved in Occator Crater on Ceres

Source: https://apod.nasa.gov/apod/ap150916.html


#CeresMystery #DawnMission #DwarfPlanet #AsteroidBelt #SpaceExploration #OccatorCrater #BrightSpots #NASA #PlanetaryScience #SpaceImage #Cosmology

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https://www.nature.com/articles/s41467-020-15973-8

https://www.nature.com/articles/s41467-020-15973-8

Fig. 1: Mapping the Bright Spots in Occator Crater
This image shows a detailed map of Occator Crater on Ceres, created using high-resolution XM2 data. The map highlights different bright areas (faculae) and estimates their thickness. Scientists used small impact craters to determine thickness—if the crater exposed dark material, the layer is thick; if it exposed bright material, the layer is thin. Black arrows point to the regions where these thickness estimates were made.

Fig. 1: Mapping the Bright Spots in Occator Crater This image shows a detailed map of Occator Crater on Ceres, created using high-resolution XM2 data. The map highlights different bright areas (faculae) and estimates their thickness. Scientists used small impact craters to determine thickness—if the crater exposed dark material, the layer is thick; if it exposed bright material, the layer is thin. Black arrows point to the regions where these thickness estimates were made.

Fig. 1: Mapping the Bright Spots in Occator Crater
This image shows a detailed map of Occator Crater on Ceres, created using high-resolution XM2 data. The map highlights different bright areas (faculae) and estimates their thickness. Scientists used small impact craters to determine thickness—if the crater exposed dark material, the layer is thick; if it exposed bright material, the layer is thin. Black arrows point to the regions where these thickness estimates were made.

Fig. 1: Mapping the Bright Spots in Occator Crater This image shows a detailed map of Occator Crater on Ceres, created using high-resolution XM2 data. The map highlights different bright areas (faculae) and estimates their thickness. Scientists used small impact craters to determine thickness—if the crater exposed dark material, the layer is thick; if it exposed bright material, the layer is thin. Black arrows point to the regions where these thickness estimates were made.

Fig. 2: Perspective views of the central region of Occator Crater.

a) This image shows a 3D-like view of Occator’s central region, highlighting important features like Cerealia Facula (bright spot), the central pit, Cerealia Tholus (a raised area), and Pasola Facula. The image is based on high-resolution data and does not exaggerate the height.

b) This image shows how the bright material (yellow and orange) relates to the lower areas (topographic lows) of Occator Crater. Yellow represents continuous bright material, orange shows less continuous bright material, and white shows other materials. The black lines show height levels, and the image is based on the digital topographic data.

Fig. 2: Perspective views of the central region of Occator Crater. a) This image shows a 3D-like view of Occator’s central region, highlighting important features like Cerealia Facula (bright spot), the central pit, Cerealia Tholus (a raised area), and Pasola Facula. The image is based on high-resolution data and does not exaggerate the height. b) This image shows how the bright material (yellow and orange) relates to the lower areas (topographic lows) of Occator Crater. Yellow represents continuous bright material, orange shows less continuous bright material, and white shows other materials. The black lines show height levels, and the image is based on the digital topographic data.

Unveiling Ceres’ bright spots ✨🔬! New research uses high-resolution images to analyze the faculae in Occator Crater, revealing how hydrothermal brines, landslides, and subsurface reservoirs shaped these unique salt deposits. 🌍🚀

#SpaceScience #Ceres #OccatorCrater #BrightSpots #Na₂CO₃ #NH₄Cl

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Preview
A Bird's Eye View of Occator Crater Dwarf planet Ceres’ Occator Crater is one of the most impressive geological structures in our solar system. New calculations by scientists at the Max Planck Institute for Solar System Research (MPS) and the University of Münster in Germany now offer the highest resolution three-dimensional reconstruction of the central depression of the Occator crater to date. With rugged slopes, circular furrows and a brilliant white central dome, the animated overflight over the inner crater area shows the whole range of geological features of this formation.

Fly over #dwarfplanetCeres' #OccatorCrater in this new 3d-animation by scientists from #MPSGoettingen and @WWU_Muenster and enjoy one of the most impressive geological formations in the Solar System. More infos here: https://t.co/0icmREYZTn and https://t.co/2bwUVv2QXc @NASA_Dawn

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