Hellas quadrangle

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

383440 characters

25 sections

221 paragraphs

200 images

322 internal links

137 external links

1. Hellas Basin

2. Lobate debris aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Upper Plains Unit

6. Climate change caused ice-rich features

7. Origin of Dao Vallis

8. Dust devil tracks

9. Evidence for possible recent liquid water

10. Other Craters

11. Glacial Features

12. Channels

13. Layers

14. Honeycomb terrain

15. Gullies

16. Polygons

17. Exposed ice sheets

18. Scalloped topography

19. Pits

20. Additional Images in Hellas quadrangle

21. Other Mars quadrangles

22. Interactive Mars map

23. See also

24. References

25. External links

hiwish 0.566

hirise 0.419

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layers 0.188

ice 0.166

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reull 0.089

tongue 0.081

terrain 0.074

layered 0.073

pits 0.068

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2017

347288 characters

24 sections

186 paragraphs

170 images

319 internal links

123 external links

1. Hellas Basin

2. Lobate debris aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Upper Plains Unit

6. Climate change caused ice-rich features

7. Origin of Dao Vallis

8. Dust devil tracks

9. Evidence for possible recent liquid water

10. Other Craters

11. Glacial Features

12. Channels

13. Layers

14. Honeycomb terrain

15. Gullies

16. Polygons

17. Scalloped topography

18. Pits

19. Additional Images in Hellas quadrangle

20. Other Mars quadrangles

21. Interactive Mars map

22. See also

23. References

24. External links

hiwish 0.562

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hellas 0.203

view 0.188

ice 0.163

layers 0.146

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polygons 0.127

close 0.110

tongue 0.096

reull 0.085

pits 0.081

terrain 0.081

dust 0.071

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2016

215231 characters

19 sections

111 paragraphs

107 images

299 internal links

38 external links

1. Hellas Basin

2. Lobate debris aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Upper Plains Unit

6. Climate change caused ice-rich features

7. Origin of Dao Vallis

8. Dust devil tracks

9. Evidence for possible recent liquid water

10. Other Craters

11. Glacial Features

12. Channels

13. Layers

14. Additional Images

15. Other Mars quadrangles

16. Interactive Mars map

17. See also

18. References

19. External links

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hirise 0.342

hellas 0.312

program 0.238

ice 0.202

glacier 0.198

reull 0.144

tongue 0.114

view 0.114

layers 0.109

tilt 0.106

layered 0.101

dust 0.095

vallis 0.091

mantle 0.091

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2015

176096 characters

17 sections

72 paragraphs

68 images

271 internal links

38 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Upper Plains Unit

6. Climate change caused ice-rich features

7. Origin of Dao Vallis

8. Dust devil tracks

9. Evidence for possible recent liquid water

10. Other Craters

11. Glacial Features

12. Channels

13. Additional Images

14. Other Mars quadrangles

15. See also

16. References

17. External links

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dust 0.125

vallis 0.121

unit 0.120

program 0.116

basin 0.111

debris 0.098

mantle 0.098

plains 0.098

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2014

146513 characters

13 sections

47 paragraphs

47 images

262 internal links

36 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Climate change caused ice-rich features

6. Origin of Dao Vallis

7. Dust devil tracks

8. Evidence for possible recent liquid water

9. Other Craters

10. Glacial Features

11. Additional Images

12. See also

13. References

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mantle 0.101

apron 0.098

image 0.095

features 0.094

debris 0.091

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2013

144357 characters

13 sections

47 paragraphs

46 images

262 internal links

36 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Climate change caused ice-rich features

6. Origin of Dao Vallis

7. Dust devil tracks

8. Evidence for possible recent liquid water

9. Other Craters

10. Glacial Features

11. Additional Images

12. See also

13. References

hellas 0.494

reull 0.252

ice 0.211

glacier 0.184

hirise 0.173

vallis 0.160

tilt 0.155

hiwish 0.139

dust 0.122

basin 0.102

mantle 0.101

apron 0.098

image 0.095

features 0.094

debris 0.091

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle, including the giant river valleys Dao Vallis, Niger Vallis, Harmakhis, and Reull Vallis—all of which may have contributed water to a lake in the Hellas basin in the distant past. [2] [3] [4] Many places in the Hellas quadrangle show signs of ice in the ground, especially places with glacier-like flow features.

2012

136127 characters

12 sections

44 paragraphs

44 images

259 internal links

36 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Origin of Dao Vallis

6. Dust devil tracks

7. Evidence for possible recent liquid water

8. Other Craters

9. Glacial Features

10. Additional Images

11. See also

12. References

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vallis 0.177

hiwish 0.154

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image 0.106

debris 0.101

water 0.099

program 0.097

dust 0.096

7152 0.089

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1]

2011

83436 characters

12 sections

43 paragraphs

37 images

112 internal links

30 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Origin of Dao Vallis

6. Dust devil tracks

7. Evidence for possible recent liquid water

8. Other Craters

9. Glacial Features

10. Additional Images

11. See also

12. References

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hirise 0.191

glacier 0.191

vallis 0.188

hiwish 0.146

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basin 0.120

apron 0.115

image 0.112

debris 0.106

water 0.105

program 0.094

lda 0.094

lobate 0.094

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1]

2010

59507 characters

11 sections

39 paragraphs

30 images

104 internal links

9 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Origin of Dao Vallis

6. Dust devil tracks

7. Evidence for possible recent liquid water

8. Other Craters

9. Additional Images

10. See also

11. References

hellas 0.507

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vallis 0.209

hirise 0.154

basin 0.134

apron 0.128

debris 0.119

water 0.117

ice 0.108

lda 0.105

lobate 0.105

dust 0.103

penticton 0.099

themis 0.096

deposits 0.096

The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program . The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1]

2009

45331 characters

10 sections

25 paragraphs

22 images

91 internal links

8 external links

1. Hellas Basin

2. Lobate Debris Aprons

3. Lineated Floor Deposits

4. Ice-rich mantle

5. Origin of Dao Vallis

6. Dust devil tracks

7. Evidence for possible recent liquid water

8. Additional Images

9. See also

10. References

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vallis 0.226

ice 0.138

lda 0.134

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water 0.132

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lineated 0.121

mantle 0.120

hadriaca 0.115

vapor 0.106

hirise 0.106

The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars . Within the Hellas quadrangle lies the classic features Hellas Planitia and Promethei Terra . Many interesting and mysterious features have been discovered in the Hellas quadrangle. Dao Vallis, a giant river valley, formed near Hadriaca Patera, an the old volcano.