Mercury (planet)

Mercury is the smallest and innermost planet in the Solar System . Its orbital period around the Sun of 87.97 days is the shortest of all the planets in the Solar System. It is named after the Roman deity Mercury , the messenger of the gods.

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

476069 characters

26 sections

86 paragraphs

57 images

814 internal links

283 external links

1. Physical characteristics

2. Orbit, rotation, and longitude

3. Observation

4. Observation history

5. Comparison

6. See also

7. Notes

8. References

9. External links

mercury 0.808

messenger 0.169

sun 0.145

caloris 0.108

planet 0.094

perihelion 0.080

magnetic 0.077

mercurian 0.076

orbit 0.068

mariner 0.067

arcseconds 0.067

solar 0.063

observations 0.063

earth 0.061

plains 0.058

Mercury is the smallest and innermost planet in the Solar System . Its orbital period around the Sun of 87.97 days is the shortest of all the planets in the Solar System. It is named after the Roman deity Mercury , the messenger of the gods.

2017

467146 characters

26 sections

83 paragraphs

57 images

814 internal links

275 external links

1. Physical characteristics

2. Orbit, rotation, and longitude

3. Observation

4. Observation history

5. Comparison

6. See also

7. Notes

8. References

9. External links

mercury 0.812

messenger 0.173

sun 0.149

caloris 0.111

planet 0.093

magnetic 0.079

mercurian 0.067

perihelion 0.067

mariner 0.065

solar 0.065

observations 0.065

earth 0.063

orbit 0.063

arcseconds 0.061

plains 0.060

Mercury is the smallest and innermost planet in the Solar System . Its orbital period around the Sun of 88 days is the shortest of all the planets in the Solar System. It is named after the Roman deity Mercury , the messenger to the gods.

2016

458402 characters

26 sections

83 paragraphs

57 images

802 internal links

252 external links

1. Physical characteristics

2. Orbit, rotation, and longitude

3. Observation

4. Observation history

5. Comparison

6. See also

7. Notes

8. References

9. External links

mercury 0.818

messenger 0.179

sun 0.150

caloris 0.110

planet 0.088

magnetic 0.078

mariner 0.068

mercurian 0.066

perihelion 0.066

earth 0.065

solar 0.064

observations 0.062

plains 0.059

orbit 0.059

orbital 0.058

Mercury is the smallest and innermost planet in the Solar System . [a] Its orbital period (about 88 Earth days) is less than any other planet in the Solar System. Seen from Earth, it appears to move around its orbit in about 116 days. It has no known natural satellites . It is named after the Roman deity Mercury , the messenger to the gods.

2015

444092 characters

24 sections

80 paragraphs

57 images

801 internal links

240 external links

1. Internal structure

2. Surface geology

3. Surface conditions and exosphere

4. Magnetic field and magnetosphere

5. Orbit, rotation, and longitude

6. Observation

7. Observation history

8. Comparison

9. See also

10. Notes

11. References

12. External links

mercury 0.823

messenger 0.172

sun 0.153

caloris 0.110

magnetic 0.097

planet 0.087

mariner 0.068

mercurian 0.066

solar 0.064

earth 0.064

observations 0.062

perihelion 0.061

plains 0.059

orbit 0.057

venus 0.057

Mercury is the smallest and closest to the Sun of the eight planets in the Solar System , [a] with an orbital period of about 88 Earth days. Seen from Earth, it appears to move around its orbit in about 116 days, which is much faster than any other planet in the Solar System. It has no known natural satellites . The planet is named after the Roman deity Mercury , the messenger to the gods.

2014

418793 characters

25 sections

85 paragraphs

42 images

812 internal links

205 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit, rotation, and longitude

6. Observation

7. Observation history

8. Comparison

9. See also

10. Notes

11. References

12. External links

mercury 0.797

sun 0.161

elongation 0.145

messenger 0.142

greatest 0.105

planet 0.105

mercurian 0.104

caloris 0.094

magnetic 0.092

equinox 0.073

mariner 0.068

earth 0.065

orbit 0.064

days 0.064

perihelion 0.063

Mercury is the smallest and closest to the Sun of the eight planets in the Solar System , [a] with an orbital period of about 88 Earth days. Seen from Earth, it appears to move around its orbit in about 116 days, which is much faster than any other planet. It has no known natural satellites . [b] The planet is named after the Roman deity Mercury , the messenger to the gods.

2013

414942 characters

23 sections

87 paragraphs

37 images

809 internal links

196 external links

1. Rotational peculiarity, and consequences

2. Internal structure

3. Surface geology

4. Surface conditions and "atmosphere" (exosphere)

5. Magnetic field and magnetosphere

6. Orbit and rotation

7. Observation

8. Observation history

9. See also

10. Notes

11. References

12. External links

mercury 0.788

sun 0.174

mercurian 0.131

elongation 0.126

messenger 0.125

planet 0.102

caloris 0.101

perihelion 0.098

greatest 0.093

magnetic 0.089

link 0.089

equinox 0.084

aphelion 0.069

sky 0.066

orbit 0.063

Mercury is the smallest and closest to the Sun of the eight planets in the Solar System , [a] with an orbital period of about 88 Earth days. Seen from the Earth, it appears to move around its orbit in about 116 days, which is much faster than any other planet. This rapid motion may have led to it being named after the Roman deity Mercury , the fast-flying messenger to the gods. Because it has almost no atmosphere to retain heat, Mercury's surface experiences the greatest temperature variation of all the planets, ranging from 100 K (−173 °C; −280 °F) at night to 700 K (427 °C; 800 °F) during the day at some equatorial regions. The poles are constantly below 180 K (−93 °C; −136 °F). Mercury's axis has the smallest tilt of any of the Solar System's planets (about ​ 130 of a degree), but it has the largest orbital eccentricity . [a] At aphelion , Mercury is about 1.5 times as far from the Sun as it is at perihelion . Mercury's surface is heavily cratered and similar in appearance to the Moon , indicating that it has been geologically inactive for billions of years.

2012

403096 characters

23 sections

85 paragraphs

36 images

800 internal links

189 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit and rotation

6. Observation

7. Observation history

8. In culture

9. See also

10. Notes

11. References

12. External links

mercury 0.798

messenger 0.142

elongation 0.137

sun 0.135

planet 0.114

caloris 0.110

greatest 0.101

magnetic 0.097

equinox 0.091

link 0.080

mariner 0.068

earth 0.065

plains 0.063

observations 0.061

basin 0.060

Mercury is the innermost planet in the Solar System . It is also the smallest, and its orbit is the most eccentric (that is, the least perfectly circular) of the eight planets. [a] It orbits the Sun once in about 88 Earth days, completing three rotations about its axis for every two orbits. The planet is named after the Roman god Mercury , the messenger to the gods.

2011

390031 characters

23 sections

75 paragraphs

38 images

798 internal links

181 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit and rotation

6. Coordinate system

7. Observation

8. Studies

9. In culture

10. See also

11. Notes

12. References

13. External links

mercury 0.796

sun 0.133

messenger 0.131

planet 0.127

caloris 0.127

magnetic 0.116

link 0.093

mariner 0.079

plains 0.077

century 0.069

basin 0.069

observations 0.068

mercurian 0.063

earth 0.063

orbit 0.063

Mercury is the innermost and smallest planet in the Solar System , [a] orbiting the Sun once every 87.969 Earth days. The orbit of Mercury has the highest eccentricity of all the Solar System planets, and it has the smallest axial tilt . It completes three rotations about its axis for every two orbits. The perihelion of Mercury's orbit precesses around the Sun at an excess of 43  arcseconds per century, a phenomenon that was explained in the 20th century by Albert Einstein 's General Theory of Relativity . [11] Mercury is bright when viewed from Earth , ranging from −2.3 to 5.7 in apparent magnitude , but is not easily seen as its greatest angular separation from the Sun is only 28.3°. Since Mercury is normally lost in the glare of the Sun, unless there is a solar eclipse it can be viewed from Earth's Northern Hemisphere only in morning or evening twilight , while its extreme elongations occur in declinations south of the celestial equator, such that it can be seen at favorable apparitions from moderate latitudes in the Southern Hemisphere in a fully dark sky.

2010

390254 characters

23 sections

73 paragraphs

34 images

838 internal links

157 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit and rotation

6. Coordinate system

7. Observation

8. Studies

9. In culture

10. See also

11. Notes

12. References

13. External links

mercury 0.790

messenger 0.143

sun 0.136

planet 0.130

caloris 0.130

magnetic 0.119

mariner 0.080

plains 0.074

century 0.071

basin 0.071

link 0.070

observations 0.069

mercurian 0.065

earth 0.065

orbit 0.065

Mercury is the innermost and smallest planet in the Solar System , [a] orbiting the Sun once every 87.969 Earth days. The orbit of Mercury has the highest eccentricity of all the Solar System planets, and it has the smallest axial tilt . It completes three rotations about its axis for every two orbits. The perihelion of Mercury's orbit precesses around the Sun at an excess of 43  arcseconds per century; a phenomenon that was explained in the 20th century by Albert Einstein 's General Theory of Relativity . [11] Mercury is bright when viewed from Earth , ranging from −2.3 to 5.7 in apparent magnitude , but is not easily seen as its greatest angular separation from the Sun is only 28.3°. Since Mercury is normally lost in the glare of the Sun, unless there is a solar eclipse it can be viewed from Earth's Northern Hemisphere only in morning or evening twilight , while its extreme elongations occur in Declinations south of the celestial equator, such that it can be seen at favorable apparitions from moderate latitudes in the Southern Hemisphere in a fully dark sky.

2009

356005 characters

23 sections

71 paragraphs

34 images

755 internal links

148 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit and rotation

6. Coordinate system

7. Observation

8. Studies of Mercury

9. Mercury in culture

10. Notes

11. See also

12. References

13. External links

mercury 0.797

messenger 0.137

caloris 0.132

sun 0.130

planet 0.128

magnetic 0.121

mariner 0.082

basin 0.077

plains 0.076

observations 0.068

mercurian 0.066

earth 0.065

solar 0.065

hermes 0.061

core 0.060

Mercury is the innermost and smallest planet in the Solar System , [9] orbiting the Sun once every 87.969 days. The orbit of Mercury has the highest eccentricity of all the Solar System planets, and it has the smallest axial tilt . It completes three rotations about the axis for every two orbits. The perihelion of Mercury's orbit precesses around the Sun at an excess of 43  arcseconds per century; a phenomenon that was explained in the 20th century by Albert Einstein 's General Theory of Relativity . [10] Mercury is bright when viewed from Earth , ranging from −2.3 to 5.7 in apparent magnitude , but is not easily seen as its greatest angular separation from the Sun is only 28.3°. Since Mercury is normally lost in the glare of the Sun, unless there is a solar eclipse , Mercury can only be viewed in morning or evening twilight .

2008

332767 characters

20 sections

66 paragraphs

36 images

788 internal links

122 external links

1. Internal structure

2. Surface geology

3. Surface conditions and "atmosphere" (exosphere)

4. Magnetic field and magnetosphere

5. Orbit and rotation

6. Observation

7. Studies of Mercury

8. Notes

9. References

10. External links

mercury 0.784

caloris 0.146

sun 0.140

planet 0.138

messenger 0.123

mariner 0.095

plains 0.084

basin 0.079

mercurian 0.073

orbit 0.073

core 0.071

magnetic 0.069

observations 0.068

earth 0.066

solar 0.060

Mercury (pronounced About this sound /ˈmɝːkjʊəri/   ) is the innermost and smallest planet in the solar system , [7] orbiting the Sun once every 88 days. Mercury is bright when viewed from Earth , ranging from −2.0 to 5.5 in apparent magnitude , but is not easily seen as its greatest angular separation from the Sun is only 28.3°. It can only be seen in morning or evening twilight . Comparatively little is known about it; the first of two spacecraft to visit Mercury was Mariner 10 , which mapped only about 45% of the planet’s surface from 1974 to 1975. The second is the MESSENGER spacecraft , which mapped another 30% during its flyby of January 14, 2008. MESSENGER will make one more pass by Mercury in 2009, followed by orbital insertion in 2011, and will then survey and map the entire planet.

2007

146430 characters

18 sections

56 paragraphs

27 images

428 internal links

33 external links

1. Internal structure

2. Surface geology

3. Atmosphere

4. Magnetosphere

5. Orbit and rotation

6. Observation

7. Studies of Mercury

8. See also

9. References

10. External links

mercury 0.775

sun 0.169

planet 0.131

caloris 0.092

mariner 0.089

orbit 0.083

core 0.072

messenger 0.072

earth 0.070

basin 0.067

resonance 0.064

magnetic 0.062

solar 0.061

venus 0.061

days 0.061

Mercury ( Template:PronEng ) is the innermost and smallest planet in the solar system , orbiting the Sun once every 88 days. It ranges in brightness from about −2.0 to 5.5 in apparent magnitude , but is not easily seen as its greatest angular separation from the Sun (greatest elongation ) is only 28.3°. It can only be seen in morning or evening twilight . Comparatively little is known about the planet: the only spacecraft to approach Mercury was Mariner 10 from 1974 to 1975, which mapped only 40%–45% of the planet’s surface.

2006

111215 characters

19 sections

55 paragraphs

22 images

375 internal links

18 external links

1. Structure

2. Orbit and rotation

3. Observation

4. Studies of Mercury

5. See also

6. References

7. External links

mercury 0.790

sun 0.164

planet 0.134

magnetic 0.096

messenger 0.085

caloris 0.075

core 0.073

orbit 0.070

perihelion 0.069

elongation 0.069

earth 0.069

resonance 0.066

mariner 0.065

venus 0.062

field 0.058

Mercury ( IPA : /ˈmɜː(r).kjʊ.ri/ ) is the innermost and smallest planet in the solar system , orbiting the Sun once every 88 days. It ranges in brightness from about −2.0 to 5.5 in apparent magnitude , but is not easily seen — its greatest angular separation from the Sun (greatest elongation ) is only 28.3° (it can only be seen in twilight ). Comparatively little is known about the planet: the only spacecraft to approach Mercury was Mariner 10 from 1974 to 1975 , which mapped only 40%–45% of the planet's surface.

2005

70922 characters

17 sections

35 paragraphs

5 images

340 internal links

8 external links

1. Historical understanding

2. Physical characteristics

3. Observing Mercury

4. Exploration

5. See also

6. Notes

7. References

8. External links

mercury 0.787

sun 0.192

planet 0.118

elongation 0.095

gm 0.086

caloris 0.078

core 0.076

orbit 0.075

earth 0.075

perihelion 0.072

greatest 0.072

velocity 0.068

messenger 0.067

twilight 0.065

eccentricity 0.064

Template:Planet Infobox/Mercury Mercury is the closest planet to the Sun , and the second-smallest planet in the Solar System . Mercury ranges from −0.4 to 5.5 in apparent magnitude , and its greatest angular separation from the Sun (greatest elongation ) is only 28.3°, meaning it is only seen in twilight . The planet remains comparatively little-known: the only spacecraft to approach Mercury was Mariner 10 from 1974 to 1975, which mapped only 40–45% of the planet's surface.

2004

77551 characters

20 sections

31 paragraphs

3 images

411 internal links

6 external links

1. Physical characteristics

2. Exploration of Mercury

3. Mercury in fiction

4. See also

5. References

6. External links

mercury 0.802

sun 0.183

elongation 0.104

mercurian 0.085

earth 0.075

velocity 0.074

core 0.074

orbit 0.073

perihelion 0.065

greatest 0.065

gu 0.063

resonance 0.062

theory 0.061

planet 0.059

magnetic 0.057

Mercury is the closest planet to the Sun , and the second-smallest planet in the solar system . Mercury ranges from –0.4 to 5.5 in apparent magnitude ; Mercury is sufficiently "close" to the Sun that telescopes rarely examine it (the greatest elongation is 28.3°). Mercury has no natural satellites . The only spacecraft to approach Mercury was Mariner 10 ( 197475 ); only 40–45% of the planet has been mapped.

2003

26703 characters

14 sections

21 paragraphs

1 images

148 internal links

3 external links

1. Physical characteristics

2. The Exploration of Mercury

3. Japan and the ESA

4. External links

5. References

mercury 0.829

sun 0.136

core 0.119

gu 0.090

theory 0.088

magnetic 0.082

mercurian 0.081

earth 0.076

perihelion 0.075

bulges 0.072

coupling 0.072

iron 0.068

velocity 0.060

locked 0.059

lasts 0.055

Mercury is the closest planet to the Sun . This is the second-smallest planet within Earth 's solar system . Upon the celestial sphere , Mercury ranges from -0.4 to 5.5, in apparent magnitude ; Mercury is sufficiently "close" to the Sun that telescopes rarely examine it. Mercury has no natural satellites . The only spacecraft to approach Mercury was Mariner 10 ( 1974 - 75 ); only 40-45% of the planet has been mapped . The astronomical symbol for Mercury is a circle on top of a short vertical line with a cross below and a semicircle above the circle.

2002

16135 characters

3 sections

16 paragraphs

1 images

77 internal links

1 external links

1. Physical characteristics

2. The exploration of Mercury

mercury 0.772

sun 0.207

caloris 0.139

perihelion 0.107

gu 0.103

magnetic 0.094

mercurian 0.093

theory 0.084

core 0.075

closest 0.071

velocity 0.069

locked 0.068

sky 0.064

resonance 0.061

continually 0.060

This mosaic of Mercury was taken by the Mariner 10 spacecraft during its approach on 29 March 1974. The mosaic consists of 18 images taken at 42 s intervals during a 13 minute period when the spacecraft was 200,000 km (about 6 hours prior to closest approach) from the planet. click here for full-sized image

2001

6344 characters

0 sections

15 paragraphs

0 images

41 internal links

0 external links

mercury 0.572

sun 0.253

locked 0.185

1350 0.140

heraclitus 0.140

tidally 0.138

caloris 0.126

rotating 0.123

colossal 0.112

resonance 0.110

sumerians 0.104

shaded 0.104

orbit 0.101

revolutions 0.101

vulcan 0.099

Mercury is the closest planet to the Sun . It has no satellites and only trace amounts of hydrogen and helium in its atmosphere (temporarily captured from the Solar wind ). Its surface appears very similar to Earth 's Moon , but the planet has a much larger iron core and is therefore much denser. Its most distinctive known surface feature is Caloris Basin, a colossal impact crater approximately 1350 km in diameter.