Solar eclipses on Mars

The two moons of Mars , Phobos and Deimos , are much smaller than the Moon , greatly reducing the frequency of solar eclipses on that planet. [1] [2] Neither moon's apparent diameter is large enough to cover the disk of the sun, and therefore they are annular solar eclipses and can also be considered transits .

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

106235 characters

5 sections

4 paragraphs

12 images

675 internal links

3 external links

1. Eclipses caused by Phobos

2. Transits caused by Deimos

3. View from Earth

4. References

5. External links

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shadow 0.199

deimos 0.175

observer 0.171

create 0.121

minutes 0.119

solar 0.111

hours 0.109

transits 0.105

cast 0.104

moons 0.104

thirty 0.102

The two moons of Mars , Phobos and Deimos , are much smaller than the Moon , greatly reducing the frequency of solar eclipses on that planet. [1] [2] Neither moon's apparent diameter is large enough to cover the disk of the sun, and therefore they are annular solar eclipses and can also be considered transits .

2017

106027 characters

5 sections

4 paragraphs

12 images

675 internal links

3 external links

1. Eclipses caused by Phobos

2. Transits caused by Deimos

3. View from Earth

4. References

5. External links

eclipses 0.471

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observer 0.172

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hours 0.110

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cast 0.105

moons 0.105

thirty 0.103

The two moons of Mars , Phobos and Deimos , are much smaller than the Moon , greatly reducing the frequency of solar eclipses on that planet. [1] [2] Neither moon's apparent diameter is large enough to cover the disk of the sun, and therefore they are annular solar eclipses and can also be considered transits .

2016

103060 characters

5 sections

5 paragraphs

12 images

673 internal links

3 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

5. External Links

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thirty 0.105

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day 0.091

The two moons of MarsPhobos and Deimos —are much smaller than the Moon, greatly reducing solar eclipses on that planet. [1] [2]

2015

102453 characters

4 sections

4 paragraphs

12 images

673 internal links

2 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

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cast 0.118

moons 0.118

thirty 0.116

small 0.102

day 0.100

The two moons of MarsPhobos and Deimos —are much smaller than the Moon, greatly reducing solar eclipses on that planet. [1] [2]

2014

102497 characters

4 sections

4 paragraphs

12 images

674 internal links

2 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

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cast 0.118

moons 0.117

thirty 0.116

small 0.102

day 0.099

The two moons of MarsPhobos and Deimos —are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet. [1] [2]

2013

102521 characters

4 sections

4 paragraphs

12 images

674 internal links

2 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

phobos 0.514

eclipses 0.396

eclipse 0.368

shadow 0.225

deimos 0.197

observer 0.193

annular 0.143

create 0.137

minutes 0.134

hours 0.123

cast 0.118

moons 0.117

thirty 0.116

small 0.102

day 0.099

The two moons of MarsPhobos and Deimos — are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet. [1] [2]

2012

92635 characters

4 sections

4 paragraphs

9 images

671 internal links

2 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

phobos 0.515

eclipses 0.397

eclipse 0.369

shadow 0.225

deimos 0.198

observer 0.193

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create 0.137

minutes 0.134

hours 0.124

cast 0.118

moons 0.118

thirty 0.116

small 0.102

The two moons of MarsPhobos and Deimos — are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet. [1] [2]

2011

92635 characters

4 sections

4 paragraphs

9 images

671 internal links

2 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

4. References

phobos 0.515

eclipses 0.397

eclipse 0.369

shadow 0.225

deimos 0.198

observer 0.193

annular 0.143

miles 0.142

create 0.137

minutes 0.134

hours 0.124

cast 0.118

moons 0.118

thirty 0.116

small 0.102

The two moons of MarsPhobos and Deimos — are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet. [1] [2]

2010

92081 characters

3 sections

4 paragraphs

10 images

676 internal links

0 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

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eclipses 0.397

eclipse 0.369

shadow 0.225

deimos 0.198

observer 0.193

annular 0.143

miles 0.142

create 0.137

minutes 0.134

hours 0.124

cast 0.118

moons 0.118

thirty 0.116

small 0.102

The two moons of MarsPhobos and Deimos — are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet.

2009

92081 characters

3 sections

4 paragraphs

10 images

676 internal links

0 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

3. View from Earth

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cast 0.118

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small 0.102

day 0.100

The two moons of MarsPhobos and Deimos — are much smaller than the Earth's moon, greatly reducing solar eclipses on that planet.

2008

90578 characters

2 sections

3 paragraphs

9 images

671 internal links

0 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

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The two moons of Mars , Phobos and Deimos are too small to cast a shadow on the planet which can be seen from Earth. However, shortly after the first artificial satellites were placed in orbit around Mars, the shadow of Phobos was seen in pictures transmitted back to Earth.

2007

7600 characters

2 sections

4 paragraphs

3 images

19 internal links

1 external links

1. Eclipses caused by Phobos

2. Eclipses caused by Deimos

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The two moons of Mars , Phobos and Deimos are too small to cast a shadow on the planet which can be seen from Earth. However, shortly after the first artificial satellites were placed in orbit around Mars, the shadow of Phobos was seen in pictures transmitted back to Earth.

2006

3627 characters

0 sections

2 paragraphs

1 images

9 internal links

0 external links

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eclipse 0.305

shadow 0.279

deimos 0.245

observer 0.239

template 0.231

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The two moons of Mars , Phobos and Deimos are too small to cast a shadow on the planet which can be seen from Earth. However, shortly after the first artificial satellites were placed in orbit around Mars, the shadow of Phobos was seen in pictures transmitted back to Earth. Because of the small size of Phobos (about 12 by 14 miles) and its rapid orbital motion, an observer on the surface of Mars would never experience a solar eclipse for longer than about twenty seconds. Because Phobos takes only 7 hours 39 minutes to orbit Mars, while a Martian day is 24 hours 37 minutes long, Phobos can create two eclipses per Martian day. Deimos is too small (about five by six miles) and too far from Mars to cause an eclipse. The best an observer on Mars would see would be a small object in transit across the Sun .