Orbital period

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun , moons orbiting planets, exoplanets orbiting other stars , or binary stars .

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

67991 characters

12 sections

25 paragraphs

3 images

176 internal links

5 external links

1. Other periods related to the orbital period

2. Small body orbiting a central body

3. Orbital period as a function of central body's density

4. Two bodies orbiting each other

5. Synodic period

6. Examples of sidereal and synodic periods

7. Binary stars

8. See also

9. Notes

10. Bibliography

11. External links

synodic 0.478

period 0.317

celestial 0.229

orbital 0.177

sidereal 0.174

body 0.166

conjunctions 0.141

periods 0.136

planets 0.133

398 0.123

p2 0.123

bodies 0.121

example 0.110

p1 0.109

m3 0.106

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun , moons orbiting planets, exoplanets orbiting other stars , or binary stars .

2017

57372 characters

10 sections

24 paragraphs

3 images

169 internal links

4 external links

1. Other periods related to the orbital period

2. Small body orbiting a central body

3. Orbital period as a function of central body's density

4. Two bodies orbiting each other

5. Synodic period

6. Examples of sidereal and synodic periods

7. Binary stars

8. See also

9. Notes

10. External links

synodic 0.424

period 0.319

celestial 0.240

orbital 0.186

sidereal 0.182

body 0.173

conjunctions 0.147

bodies 0.144

398 0.129

p2 0.129

periods 0.122

example 0.115

p1 0.115

m3 0.111

ρ 0.110

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun , moons orbiting planets, exoplanets orbiting other stars , or binary stars .

2016

53686 characters

10 sections

21 paragraphs

3 images

160 internal links

3 external links

1. Periods related to the orbital period

2. Small body orbiting a central body

3. Orbital period as a function of central body's density

4. Two bodies orbiting each other

5. Synodic period

6. Examples of sidereal and synodic periods

7. Binary stars

8. See also

9. Notes

10. External links

synodic 0.356

period 0.286

orbital 0.238

body 0.218

citation 0.210

p2 0.198

p1 0.176

m3 0.171

ρ 0.169

periods 0.157

needed 0.152

orbit 0.143

unit 0.141

sidereal 0.140

completing 0.117

The orbital period is the time taken for a given object to make one complete orbit around another object.

2015

60720 characters

10 sections

17 paragraphs

2 images

147 internal links

2 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Binary stars

4. See also

5. Notes

6. External links

p_ 0.400

synodic 0.324

displaystyle 0.321

ρ 0.309

period 0.242

orbital 0.196

rho 0.180

m3 0.156

citation 0.137

body 0.133

unit 0.129

sidereal 0.128

periods 0.114

universal 0.104

bodies 0.101

The orbital period is the time taken for a given object to make one complete orbit around another object.

2014

67974 characters

11 sections

19 paragraphs

2 images

149 internal links

2 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. See also

6. Notes

7. External links

displaystyle 0.403

p_ 0.376

synodic 0.305

ρ 0.291

period 0.263

orbital 0.184

rho 0.170

m3 0.147

citation 0.129

body 0.125

unit 0.121

sidereal 0.120

periods 0.107

semi 0.099

universal 0.098

The orbital period is the time taken for a given object to make one complete orbit around another object.

2013

61488 characters

11 sections

17 paragraphs

2 images

150 internal links

0 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. See also

6. Notes

7. External links

p_ 0.428

synodic 0.347

displaystyle 0.286

period 0.259

orbital 0.209

citation 0.205

m3 0.167

ρ 0.165

needed 0.149

body 0.142

unit 0.138

sidereal 0.137

periods 0.122

universal 0.111

bodies 0.108

The orbital period is the time taken for a given object to make one complete orbit around another object.

2012

55497 characters

9 sections

16 paragraphs

2 images

148 internal links

0 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. See also

6. Notes

citation 0.339

synodic 0.297

period 0.282

needed 0.246

orbital 0.209

unit 0.177

sidereal 0.175

body 0.152

displaystyle 0.147

universal 0.143

2624 0.137

2648 0.124

deimos 0.123

observer 0.120

ellipses 0.116

The orbital period is the time taken for a given object to make one complete orbit about another object.

2011

56455 characters

9 sections

18 paragraphs

2 images

148 internal links

0 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. Notes

6. See also

citation 0.374

synodic 0.295

period 0.280

needed 0.271

body 0.242

orbital 0.208

sidereal 0.174

displaystyle 0.146

universal 0.142

2624 0.136

2648 0.123

deimos 0.123

observer 0.120

ellipses 0.115

spherically 0.115

The orbital period is the time taken for a given object to make one complete orbit about another object.

2010

60125 characters

8 sections

28 paragraphs

2 images

149 internal links

0 external links

1. Relation between the sidereal and synodic periods

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. See also

synodic 0.406

sidereal 0.342

period 0.319

body 0.190

angular 0.170

orbital 0.163

inferior 0.155

object 0.150

planet 0.119

displaystyle 0.115

universal 0.112

superior 0.111

velocity 0.108

2624 0.107

360 0.103

The orbital period is the time taken for a given object to make one complete orbit about another object.

2009

59876 characters

8 sections

28 paragraphs

2 images

148 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

3. Tangential velocities at altitude

4. Binary stars

5. See also

synodic 0.406

sidereal 0.342

period 0.320

body 0.190

angular 0.170

orbital 0.163

inferior 0.156

object 0.150

planet 0.119

displaystyle 0.115

universal 0.112

superior 0.111

velocity 0.108

2624 0.107

360 0.103

The orbital period is the time taken for a given object to make one complete orbit about another object.

2008

56867 characters

7 sections

28 paragraphs

1 images

145 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

3. Tangential velocities at altitude

4. See also

synodic 0.409

sidereal 0.345

period 0.322

body 0.191

angular 0.172

orbital 0.164

inferior 0.157

object 0.151

planet 0.119

displaystyle 0.116

universal 0.112

superior 0.111

velocity 0.109

2624 0.108

360 0.104

The orbital period is the time taken for a given object to make one complete orbit about another object.

2007

57768 characters

7 sections

28 paragraphs

1 images

145 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

3. Tangential velocities at altitude

4. See also

synodic 0.410

sidereal 0.346

period 0.323

body 0.192

angular 0.172

orbital 0.165

inferior 0.157

object 0.152

planet 0.120

displaystyle 0.116

universal 0.113

superior 0.112

velocity 0.109

2624 0.108

360 0.104

The orbital period is the time taken for a given object to make one complete orbit about another object.

2006

36316 characters

5 sections

27 paragraphs

0 images

51 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

synodic 0.429

period 0.317

sidereal 0.289

body 0.201

angular 0.180

orbital 0.173

inferior 0.164

planet 0.138

displaystyle 0.121

universal 0.118

superior 0.117

velocity 0.114

2624 0.113

360 0.109

formulae 0.102

Copernicus devised a mathematical formula to calculate a planet's sidereal period from its synodic period.

2005

32496 characters

5 sections

25 paragraphs

0 images

46 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

synodic 0.405

period 0.303

sidereal 0.239

body 0.221

angular 0.199

orbital 0.190

displaystyle 0.134

universal 0.130

velocity 0.126

2624 0.125

360 0.120

2648 0.113

deimos 0.112

planet 0.111

observer 0.109

Copernicus devised a mathematical formula to calculate a planet's sidereal period from its synodic period.

2004

31723 characters

5 sections

24 paragraphs

0 images

42 internal links

0 external links

1. Relation between sidereal and synodic period

2. Calculation

body 0.269

period 0.255

synodic 0.246

angular 0.241

orbital 0.231

sidereal 0.194

displaystyle 0.163

universal 0.158

velocity 0.153

360 0.146

orbit 0.132

full 0.132

algebra 0.128

ellipses 0.128

spherically 0.128

Copernicus devised a mathematical formula to calculate a planet's sidereal period from its synodic period.

2003

3543 characters

2 sections

8 paragraphs

0 images

14 internal links

0 external links

1. Relation between sidereal and synodic period

360 0.294

toe 0.276

algebra 0.259

moves 0.249

abbreviations 0.229

inferior 0.222

relate 0.207

planet 0.203

sidereal 0.195

devised 0.184

copernicus 0.181

period 0.171

likewise 0.167

synodic 0.165

derives 0.164

Copernicus devised a mathematical formula to relate a planet's sidereal period with its synodic period.

2002

2949 characters

1 sections

15 paragraphs

0 images

10 internal links

0 external links

1. History of the Orbital Period

sidereal 0.539

period 0.378

synodic 0.366

092 0.338

object 0.189

orbital 0.147

algebra 0.143

years 0.127

inferior 0.123

takes 0.119

relate 0.114

planet 0.112

1 0.112

configurations 0.106

devised 0.102

The sidereal period is the time that it takes for the object to make one full orbit, relative to the stars. This is considered to be an object's true orbital period.