Kipini (crater)

Kipini is an impact crater in the Oxia Palus quadrangle of Mars . It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

77294 characters

2 sections

3 paragraphs

5 images

659 internal links

4 external links

1. See also

2. References

kipini 0.626

kenya 0.279

craters 0.223

ejecta 0.217

peak 0.198

rim 0.165

ratios 0.157

oxia 0.155

rebound 0.153

crater 0.140

town 0.139

relationship 0.130

deal 0.125

impact 0.122

palus 0.121

Kipini is an impact crater in the Oxia Palus quadrangle of Mars . It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

2017

35911 characters

2 sections

3 paragraphs

8 images

165 internal links

4 external links

1. See also

2. References

kipini 0.626

kenya 0.279

craters 0.223

ejecta 0.217

peak 0.198

rim 0.165

ratios 0.157

oxia 0.155

rebound 0.153

crater 0.140

town 0.139

relationship 0.130

deal 0.125

impact 0.122

palus 0.121

Kipini is an impact crater in the Oxia Palus quadrangle of Mars . It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

2016

35454 characters

3 sections

5 paragraphs

8 images

161 internal links

4 external links

1. Why are Craters important?

2. See also

3. References

kipini 0.454

craters 0.324

kenya 0.203

deposits 0.177

impact 0.177

ice 0.170

dissolves 0.164

ores 0.161

ejecta 0.157

crater 0.152

melts 0.147

ore 0.145

peak 0.143

minerals 0.140

rich 0.127

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

2015

35452 characters

3 sections

5 paragraphs

8 images

161 internal links

4 external links

1. Why are Craters important?

2. See also

3. References

kipini 0.454

craters 0.324

kenya 0.203

deposits 0.177

impact 0.177

ice 0.170

dissolves 0.164

ores 0.161

ejecta 0.157

crater 0.152

melts 0.147

ore 0.145

peak 0.143

minerals 0.140

rich 0.127

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

2014

34938 characters

3 sections

5 paragraphs

8 images

161 internal links

4 external links

1. Why are Craters important?

2. See also

3. References

kipini 0.454

craters 0.324

kenya 0.203

deposits 0.177

impact 0.177

ice 0.170

dissolves 0.164

ores 0.161

ejecta 0.157

crater 0.152

melts 0.147

ore 0.145

peak 0.143

minerals 0.140

rich 0.127

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different. [4]

2013

27571 characters

1 sections

2 paragraphs

7 images

157 internal links

1 external links

1. References

kipini 0.607

kenya 0.541

oxia 0.300

town 0.269

palus 0.234

31 0.206

26 0.173

crater 0.135

6 0.089

quadrangle 0.083

impact 0.079

located 0.067

1 0.056

named 0.045

mars 0.017

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1]

2011

6259 characters

1 sections

2 paragraphs

3 images

12 internal links

1 external links

1. References

kipini 0.607

kenya 0.541

oxia 0.300

town 0.269

palus 0.234

31 0.206

26 0.173

crater 0.135

6 0.089

quadrangle 0.083

impact 0.079

located 0.067

1 0.056

named 0.045

mars 0.017

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1]

2010

5805 characters

1 sections

2 paragraphs

3 images

8 internal links

1 external links

1. References

kipini 0.798

kenya 0.356

oxia 0.197

town 0.177

bar 0.155

palus 0.154

31 0.135

crater 0.134

26 0.114

rim 0.105

scale 0.105

meters 0.097

500 0.091

hirise 0.090

south 0.069

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1° N and 31.6° W It is named after a Town in Kenya. [1]

2009

5793 characters

1 sections

2 paragraphs

3 images

8 internal links

1 external links

1. References

kipini 0.798

kenya 0.356

oxia 0.197

town 0.177

bar 0.155

palus 0.154

31 0.135

crater 0.134

26 0.114

rim 0.105

scale 0.105

meters 0.097

500 0.091

hirise 0.090

south 0.069

Kipini Crater is an impact crater in the Oxia Palus quadrangle of Mars. It is located at 26.1 N and 31.6 W It is named after a Town in Kenya. [1]