Ring mold crater

A Ring mold crater is a kind of crater on the planet Mars that looks like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in lobate debris aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

80861 characters

3 sections

16 paragraphs

13 images

643 internal links

1 external links

1. See also

2. References

3. External links

mold 0.772

ring 0.429

hiwish 0.210

hirise 0.150

craters 0.138

ice 0.135

program 0.111

ismenius 0.092

view 0.082

lacus 0.080

undergoes 0.071

shape 0.063

crater 0.056

debris 0.054

image 0.050

A Ring mold crater is a kind of crater on the planet Mars that looks like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in lobate debris aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2017

38859 characters

3 sections

15 paragraphs

16 images

151 internal links

1 external links

1. See also

2. References

3. External links

mold 0.766

ring 0.427

hiwish 0.220

hirise 0.157

craters 0.145

ice 0.130

program 0.116

ismenius 0.096

view 0.086

lacus 0.083

undergoes 0.074

shape 0.066

debris 0.056

image 0.053

crater 0.052

Ring Mold Craters are a kind of crater on the planet Mars , that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in lobate debris aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2016

33525 characters

3 sections

9 paragraphs

10 images

150 internal links

1 external links

1. See also

2. References

3. External links

mold 0.742

ring 0.424

ice 0.189

hiwish 0.145

craters 0.135

hirise 0.114

undergoes 0.108

shape 0.095

ismenius 0.093

debris 0.082

lacus 0.081

image 0.077

program 0.077

baking 0.070

insulate 0.070

Ring Mold Craters are a kind of crater on the planet Mars , that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in lobate debris aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2015

34991 characters

3 sections

9 paragraphs

11 images

154 internal links

1 external links

1. See also

2. References

3. External links

mold 0.742

ring 0.424

ice 0.189

hiwish 0.145

craters 0.135

hirise 0.114

undergoes 0.108

shape 0.095

ismenius 0.093

debris 0.082

lacus 0.081

image 0.077

program 0.077

baking 0.070

insulate 0.070

Ring Mold Craters are a kind of crater on the planet Mars , that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in Lobate Debris Aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2013

8564 characters

2 sections

5 paragraphs

4 images

12 internal links

0 external links

1. References

2. See also

mold 0.657

ring 0.405

ice 0.279

shape 0.169

debris 0.144

baking 0.124

insulate 0.124

molds 0.120

mamers 0.120

image 0.109

footprint 0.107

craters 0.106

impacts 0.099

deuteronilus 0.093

lineated 0.089

Ring Mold Craters are kind of crater on the planet Mars , that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in Lobate Debris Aprons and lineated valley fill . Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2011

5382 characters

1 sections

3 paragraphs

2 images

5 internal links

0 external links

1. References

mold 0.573

ring 0.378

ice 0.292

shape 0.165

baking 0.162

molds 0.157

mamers 0.157

image 0.142

footprint 0.141

impacts 0.130

debris 0.126

deuteronilus 0.122

lineated 0.117

dichotomy 0.116

mensae 0.109

Ring Mold Craters are kind of crater on the planet Mars , that look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in Lobate Debris Aprons and lineated valley fill. Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.

2010

5571 characters

2 sections

3 paragraphs

2 images

3 internal links

0 external links

1. Ring Mold Craters

2. References

mold 0.576

ring 0.380

ice 0.294

shape 0.166

baking 0.163

molds 0.158

mamers 0.158

image 0.143

footprint 0.141

impacts 0.130

debris 0.127

deuteronilus 0.123

lineated 0.118

dichotomy 0.117

mensae 0.109

Ring Mold Craters look like the ring molds used in baking. They are believed to be caused by an impact into ice. The ice is covered by a layer of debris. They are found in parts of Mars that have buried ice. Laboratory experiments confirm that impacts into ice result in a "ring mold shape." They are also bigger than other craters in which an asteroid impacted solid rock. Impacts into ice warm the ice and cause it to flow into the ring mold shape. These craters are common in Lobate Debris Aprons and lineated valley fill. Many have been found in Mamers Valles , a channel found along the dichotomy boundary in Deuteronilus Mensae . [1] [2] [3] They may be an easy way for future colonists of Mars to find water ice.