Mare Australe quadrangle

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2] The Mars polar lander crash landed in this region. [3] [4]

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

206735 characters

19 sections

114 paragraphs

99 images

298 internal links

34 external links

1. Notable features

2. Freezing of atmosphere

3. Lake of liquid water

4. Spiders

5. Defrosting

6. Dust devil tracks

7. Dorsa Argentea Formation

8. Proof for ocean

9. Craters

10. Craters showing layers

11. Craters showing defrosting in spring

12. Polygons

13. Swiss Cheese Terrain

14. Other features in Mare Australe quadrangle

15. Other Mars quadrangles

16. Interactive Mars map

17. See also

18. References

19. External links

ctx 0.282

reconnaissance 0.217

camera 0.214

hiwish 0.206

hirise 0.200

spiders 0.188

crater 0.187

frost 0.175

defrosting 0.162

orbiter 0.158

ice 0.157

dust 0.153

dark 0.152

enlargement 0.146

eskers 0.141

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2] The Mars polar lander crash landed in this region. [3] [4]

2017

198054 characters

17 sections

106 paragraphs

94 images

295 internal links

33 external links

1. Notable features

2. Freezing of atmosphere

3. Spiders

4. Defrosting

5. Dust devil tracks

6. Dorsa Argentea Formation

7. Proof for ocean

8. Craters

9. Craters showing layers

10. Craters showing defrosting in spring

11. Swiss Cheese Terrain

12. Other features in Mare Australe quadrangle

13. Other Mars quadrangles

14. Interactive Mars map

15. See also

16. References

17. External links

ctx 0.296

reconnaissance 0.228

camera 0.224

spiders 0.197

crater 0.194

hirise 0.183

hiwish 0.176

defrosting 0.170

orbiter 0.166

dust 0.161

dark 0.160

enlargement 0.153

eskers 0.148

ice 0.148

frost 0.145

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2] The Mars polar lander crash landed in this region. [3] [4]

2016

162494 characters

16 sections

80 paragraphs

78 images

286 internal links

18 external links

1. Notable features

2. Freezing of atmosphere

3. Spiders

4. Defrosting

5. Dorsa Argentea Formation

6. Proof for ocean

7. Craters

8. Dust devil tracks

9. Craters showing layers

10. Craters showing defrosting in spring

11. Gallery

12. Other Mars quadrangles

13. Interactive Mars map

14. See also

15. References

16. External links

ctx 0.349

reconnaissance 0.268

camera 0.252

crater 0.226

defrosting 0.200

orbiter 0.190

enlargement 0.180

dark 0.176

frost 0.159

eskers 0.155

dust 0.142

note 0.138

devil 0.133

cheese 0.126

lyell 0.122

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2] The Mars polar lander crash landed in this region. [3] [4]

2015

140446 characters

11 sections

68 paragraphs

69 images

254 internal links

14 external links

1. Notable features

2. Gallery

3. Spiders

4. Proof for ocean

5. Craters

6. Dust devil tracks

7. Craters showing layers

8. Craters showing defrosting in spring

9. Other Mars quadrangles

10. See also

11. References

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camera 0.277

crater 0.248

orbiter 0.209

enlargement 0.198

frost 0.175

note 0.152

devil 0.147

cheese 0.138

dark 0.138

lyell 0.134

previous 0.132

image 0.131

dust 0.130

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2]

2014

86955 characters

4 sections

21 paragraphs

26 images

227 internal links

7 external links

1. Notable features

2. Gallery

3. See also

4. References

cheese 0.319

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hirise 0.258

australe 0.222

angustus 0.208

spider 0.205

devil 0.203

inca 0.186

cavi 0.159

burst 0.133

cap 0.133

labyrinthus 0.132

surveyor 0.129

mare 0.128

polygonal 0.117

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2]

2013

86122 characters

4 sections

21 paragraphs

25 images

227 internal links

7 external links

1. Notable features

2. Gallery

3. See also

4. References

cheese 0.319

swiss 0.281

hirise 0.258

australe 0.222

angustus 0.208

spider 0.205

devil 0.203

inca 0.186

cavi 0.159

burst 0.133

cap 0.133

labyrinthus 0.132

surveyor 0.129

mare 0.128

polygonal 0.117

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2]

2012

83816 characters

4 sections

21 paragraphs

23 images

227 internal links

7 external links

1. Notable features

2. Gallery

3. See also

4. References

cheese 0.319

swiss 0.281

hirise 0.258

australe 0.222

angustus 0.208

spider 0.205

devil 0.203

inca 0.186

cavi 0.159

burst 0.133

cap 0.133

labyrinthus 0.132

surveyor 0.129

mare 0.128

polygonal 0.117

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap , and its surrounding area. The quadrangle's name derives from an older name for a feature that is now called Planum Australe , a large plain surrounding the polar cap. [2]

2011

62058 characters

10 sections

31 paragraphs

18 images

91 internal links

20 external links

1. Inca City

2. Ice Cap

3. Misplaced Ice Cap

4. Swiss Cheese appearance

5. Mars is getting warmer?

6. Layers

7. Starburst Channels (Spiders)

8. Other Features in the Mare Australe quadrangle

9. See also

10. References

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spiders 0.173

swiss 0.165

dust 0.158

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polar 0.149

hirise 0.132

gas 0.131

pole 0.131

inca 0.131

south 0.127

dioxide 0.118

retreat 0.115

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The Mare Australe quadrangle covers all the area of Mars south of 65°. Around the southern ice cap is a surface, called the Dorsa Argentea Formation that may be an old ice-rich deposit. It contains a group of sinuous, branched ridges that resembles eskers that form when streams are under glaciers. [2] The formation often contains pits: two major locations are named Cavi Angusti and Cavi Sisyphi. The pits have steep sides and an irregular shape. They are up to 50 km across and 1 km deep. [3]

2010

48145 characters

10 sections

31 paragraphs

18 images

85 internal links

7 external links

1. Inca City

2. Ice Cap

3. Misplaced Ice Cap

4. Swiss Cheese appearance

5. Mars is getting warmer?

6. Layers

7. Starburst Channels (Spiders)

8. Other Features in the Mare Australe quadrangle

9. See also

10. References

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ice 0.240

cheese 0.227

spiders 0.175

swiss 0.167

dust 0.161

australe 0.158

polar 0.151

hirise 0.134

gas 0.133

inca 0.132

south 0.120

retreat 0.116

pole 0.116

pits 0.105

The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The Mare Australe quadrangle covers all the area of Mars south of 65°. Around the southern ice cap is a surface, called the Dorsa Argentea Formation that may be an old ice-rich deposit. It contains a group of sinuous, branched ridges that resembles eskers that form when streams are under glaciers. [2] The formation often contains pits: two major locations are named Cavi Angusti and Cavi Sisyphi. The pits have steep sides and an irregular shape. They are up to 50 km across and 1 km deep. [3]

2009

37636 characters

10 sections

25 paragraphs

16 images

79 internal links

6 external links

1. Inca City

2. Ice Cap

3. Misplaced Ice Cap

4. Swiss Cheese appearance

5. Mars is getting warmer?

6. Layers

7. Starburst Channels (Spiders)

8. Gallery

9. See also

10. References

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ice 0.206

inca 0.173

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snow 0.131

pole 0.130

devil 0.126

dust 0.126

polar 0.126

south 0.123

walls 0.114

Mariner 9 showed a small area located at 82° S and 66° W that looked like the ruins of an ancient city. Mariner 9 team members named it "Inca City." It looked like sand dunes that formed from winds that blew from two different directions, but the dunes were too big. In 2002 the camera on Mars Global Surveyor revealed that Inca City was part of a large circular structure that was 86 km in diameter. So the shape meant that it was probably caused by an asteroid impact which cracked the crust. Later, magma flowed along the cracks. When the magma cooled, hard, erosion resistant walls of rock (dikes) formed. The crater was covered over, then partially exhumed. The hard walls of rock wre left standing as softer surrounding material eroded away. [1]