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Sun-synchronous orbit

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2806: 90: 2818: 22: 887: 2890: 2780: 1199:
maximum for a Sun-synchronous orbit, and doing more than 16 would require an orbit inside the Earth's atmosphere or surface. The resulting valid orbits are shown in the following table. (The table has been calculated assuming the periods given. The orbital period that should be used is actually slightly longer. For instance, a retrograde equatorial orbit that passes over the same spot after 24 hours has a true period about
2854: 2878: 2830: 596: 2866: 2842: 1095: 882:{\displaystyle {\begin{aligned}\rho &\approx -{\frac {3J_{2}R_{\text{E}}^{2}{\sqrt {\mu }}\cos i}{2a^{7/2}}}\\&=-(360^{\circ }{\text{ per year}})\times \left({\frac {a}{12\,352{\text{ km}}}}\right)^{-7/2}\cos i\\&=-(360^{\circ }{\text{ per year}})\times \left({\frac {T}{3.795{\text{ h}}}}\right)^{-7/3}\cos i,\end{aligned}}} 121:
between day and night. Riding the terminator is useful for active radar satellites, as the satellites' solar panels can always see the Sun, without being shadowed by the Earth. It is also useful for some satellites with passive instruments that need to limit the Sun's influence on the measurements,
85:
wavelengths, such as weather and spy satellites, and for other remote-sensing satellites, such as those carrying ocean and atmospheric remote-sensing instruments that require sunlight. For example, a satellite in Sun-synchronous orbit might ascend across the equator twelve times a day, each time at
1628:
evolve, due to higher-order perturbations in the Earth's gravitational field, the pressure of sunlight, and other causes. Earth observation satellites, in particular, prefer orbits with constant altitude when passing over the same spot. Careful selection of eccentricity and location of perigee
1198:
If one wants a satellite to fly over some given spot on Earth every day at the same hour, the satellite must complete a whole number of orbits per day. Assuming a circular orbit, this comes down to between 7 and 16 orbits per day, as doing less than 7 orbits would require an altitude above the
902: 170:, which perturbs inclined orbits, causes the orbital plane of the spacecraft to precess with the desired rate. The plane of the orbit is not fixed in space relative to the distant stars, but rotates slowly about the Earth's axis. 297: 25:
Diagram showing the orientation of a Sun-synchronous orbit (green) at four points in the year. A non-Sun-synchronous orbit (magenta) is also shown for reference. Dates are shown in white: day/month.
1090:{\displaystyle \cos i\approx -{\frac {2\rho }{3J_{2}R_{\text{E}}^{2}{\sqrt {\mu }}}}a^{7/2}=-\left({\frac {a}{12\,352{\text{ km}}}}\right)^{7/2}=-\left({\frac {T}{3.795{\text{ h}}}}\right)^{7/3}.} 551: 601: 1722: 214: 1629:
reveals specific combinations where the rate of change of perturbations are minimized, and hence the orbit is relatively stable – a
1960: 1781: 122:
as it is possible to always point the instruments towards the night side of the Earth. The dawn/dusk orbit has been used for solar-observing
1742: 1671: 1143:, which means that only lower orbits can be Sun-synchronous. The period can be in the range from 88 minutes for a very low orbit ( 105:
of 10:30. The LST zones show how the local time beneath the satellite varies at different latitudes and different points on its orbit.
117:, where the local mean solar time of passage for equatorial latitudes is around sunrise or sunset, so that the satellite rides the 173:
Typical Sun-synchronous orbits around Earth are about 600–800 km (370–500 mi) in altitude, with periods in the 96–100-
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Low, Samuel Y. W. (January 2022). "Designing a Reference Trajectory for Frozen Repeat Near-Equatorial Low Earth Orbits".
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compared to the direction of Earth's rotation: 0° represents an equatorial orbit, and 90° represents a polar orbit.
2712: 2592: 2011: 569: 2805: 2677: 2431: 2750: 2389: 2380: 2117: 1947: 1215:≈ 1.0027 times longer than the time between overpasses. For non-equatorial orbits the factor is closer to 1.) 45:
around a planet, in which the satellite passes over any given point of the planet's surface at the same local
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over the Earth surface. Even if an orbit remains Sun-synchronous, however, other orbital parameters such as
2697: 2167: 113:, where the local mean solar time of passage for equatorial latitudes is around noon or midnight, and the 2642: 1613: 1967: 77:
on the planet underneath it is nearly the same. This consistent lighting is a useful characteristic for
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through one complete revolution each year, so it always maintains the same relationship with the Sun.
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of the spacecraft over Earth's surface, this formula gives a Sun-synchronous inclination of 98.7°.
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Rosengren, M. (November 1992). "ERS-1 - An Earth Observer that exactly follows its Chosen Path".
1601:. The Sun will not be in exactly the same position in the sky during the course of the year (see 2617: 2219: 2139: 2127: 1819: 1723:"Stabilization of heliosynchronous orbits of an Earth's artificial satellite by solar pressure" 1171:= 180°). A period longer than 3.8 hours may be possible by using an eccentric orbit with 352: 2910: 2740: 2682: 2652: 2440: 2285: 2255: 2199: 2078: 1701: 1658: 1642: 1621: 123: 1916:
Rosengren, Mats (1989). "Improved technique for Passive Eccentricity Control (AAS 89-155)".
1811: 1764: 2765: 2587: 2371: 2260: 2229: 2157: 2132: 2107: 2068: 2049: 2004: 1921: 1882: 1855: 1734: 1681: 1625: 162:. This precession is achieved by tuning the inclination to the altitude of the orbit (see 8: 2882: 2627: 2422: 2162: 1686: 1598: 1925: 1886: 1859: 1738: 196:
that is almost spherical will need an outside push to maintain a Sun-synchronous orbit.
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When one says that a Sun-synchronous orbit goes over a spot on the Earth at the same
178: 70: 62: 2834: 2647: 2579: 2343: 2305: 2179: 2149: 2102: 1890: 1602: 205: 167: 155: 151: 147: 292:{\displaystyle \Delta \Omega =-3\pi {\frac {J_{2}R_{\text{E}}^{2}}{p^{2}}}\cos i,} 2687: 2280: 2184: 2174: 2073: 1997: 1594: 561: 185: 46: 2894: 2810: 2783: 2735: 2727: 2722: 2607: 2602: 2533: 2513: 2504: 2097: 2083: 2059: 2054: 2029: 1691: 2904: 2637: 2632: 2551: 2194: 2112: 403: 2846: 2702: 2612: 2486: 2469: 2327: 2224: 2092: 1630: 102: 2707: 2542: 2312: 2292: 2209: 1696: 42: 21: 154:(rotate) approximately one degree eastward each day with respect to the 2275: 1989: 1654: 330: 98: 50: 2889: 2692: 2044: 1894: 78: 208:
per orbit for an Earth orbiting satellite is approximately given by
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Sandwell, David T., The Gravity Field of the Earth - Part 1 (2002)
2597: 1638: 135: 73:, because every time that the satellite is overhead, the surface 1633:, where the motion of position of the periapsis is stable. The 419: 174: 1721:
Tscherbakova, N. N.; Beletskii, V. V.; Sazonov, V. V. (1999).
2402: 2021: 1646: 193: 127: 1720: 1229: 189: 2841: 1818:(1st ed.). Cambridge University Press. 2007. p.  1661:, are all operated in such Sun-synchronous frozen orbits. 365:
An orbit will be Sun-synchronous when the precession rate
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for a circular or almost circular orbit, it follows that
159: 177:
range, and inclinations of around 98°. This is slightly
49:. More technically, it is an orbit arranged so that it 138:, affording them a nearly continuous view of the Sun. 2794: 905: 599: 546:{\displaystyle T=2\pi {\sqrt {\frac {a^{3}}{\mu }}},} 508: 217: 1966:. Space Flight Mechanics Conference. Archived from 109:Special cases of the Sun-synchronous orbit are the 1089: 881: 545: 496:is the period of the spacecraft around the earth. 393:equals the mean motion of the Earth about the Sun 291: 158:to keep pace with the Earth's movement around the 146:A Sun-synchronous orbit is achieved by having the 184:Sun-synchronous orbits are possible around other 2902: 1612:Sun-synchronous orbits are mostly selected for 361:is the inclination of the orbit to the equator. 2005: 1616:, with an altitude typically between 600 and 93:Sun-synchronous orbit from a top view of the 81:that image the Earth's surface in visible or 1961:"The A-B-Cs of Sun Synchronous Orbit Design" 1985:List of satellites in Sun-synchronous orbit 1950:, from U.S. Centennial of Flight Commission 1714: 1167:, but this orbit would be equatorial, with 2779: 2012: 1998: 1672:Orbital perturbation analysis (spacecraft) 1135:equals −1 when the semi-major axis equals 1128:Note that according to this approximation 1915: 1845: 1008: 741: 499:As the orbital period of a spacecraft is 2019: 1814:Our Changing Planet: The View from Space 192:. A satellite orbiting a planet such as 88: 20: 2903: 2658:Transposition, docking, and extraction 1948:Sun-Synchronous Orbit dictionary entry 1918:Advances in the Astronautical Sciences 1875:AIAA Journal of Spacecraft and Rockets 163: 61:A Sun-synchronous orbit is useful for 1993: 1958: 327:coefficient for the second zonal term 141: 86:approximately 15:00 mean local time. 1841: 1839: 199: 1872: 13: 1959:Boain, Ronald J. (February 2004). 1935: 492:is the earth orbital period while 221: 218: 14: 2922: 2718:Kepler's laws of planetary motion 1978: 1854:(72). European Space Agency: 76. 1836: 1804: 2888: 2876: 2864: 2852: 2840: 2828: 2816: 2804: 2778: 2713:Interplanetary Transport Network 2593:Collision avoidance (spacecraft) 570:standard gravitational parameter 345:is the mean radius of the Earth, 101:(LST) zones for reference and a 2678:Astronomical coordinate systems 2432:Longitude of the ascending node 56: 2751:Retrograde and prograde motion 1909: 1866: 1774: 1757: 814: 796: 721: 703: 1: 1708: 2698:Equatorial coordinate system 1614:Earth observation satellites 7: 1664: 10: 2927: 2450:Longitude of the periapsis 1920:. Vol. 69. AAS/NASA. 1593:each time, this refers to 1155:= 96°) to 3.8 hours ( 2774: 2761:Specific angular momentum 2666: 2578: 2522: 2458: 2411: 2351: 2342: 2238: 2148: 2037: 2028: 1227: 1108:, i.e., for an altitude 16:Type of geocentric orbit 2756:Specific orbital energy 1765:"SATELLITES AND ORBITS" 2168:Geostationary transfer 1091: 883: 547: 293: 106: 39:heliosynchronous orbit 26: 2741:Orbital state vectors 2683:Characteristic energy 2653:Trans-lunar injection 2441:Argument of periapsis 2118:Prograde / Retrograde 2079:Hyperbolic trajectory 1702:World Geodetic System 1659:Canadian Space Agency 1643:European Space Agency 1622:argument of periapsis 1092: 884: 548: 294: 124:scientific satellites 92: 31:Sun-synchronous orbit 24: 2588:Bi-elliptic transfer 2108:Parabolic trajectory 1682:Geosynchronous orbit 1626:orbital eccentricity 1100:As an example, with 903: 597: 506: 402:, which is 360° per 215: 166:) such that Earth's 2628:Low-energy transfer 1973:on 25 October 2007. 1926:1989ommd.proc...49R 1887:2022JSpRo..59...84L 1860:1992ESABu..72...76R 1739:1999KosIs..37..417S 1687:Geostationary orbit 1599:apparent solar time 959: 647: 263: 111:noon/midnight orbit 2623:Inclination change 2271:Distant retrograde 1786:marine.rutgers.edu 1087: 945: 896:is 360° per year, 879: 877: 633: 564:of the orbit, and 543: 424:), so we must set 289: 249: 142:Orbital precession 107: 75:illumination angle 71:weather satellites 27: 2792: 2791: 2766:Two-line elements 2574: 2573: 2496:Eccentric anomaly 2338: 2337: 2205:Orbit of the Moon 2064:Highly elliptical 1792:on 22 August 2019 1782:"Types of Orbits" 1645:, as well as the 1585: 1584: 1064: 1061: 1018: 1015: 968: 965: 952: 840: 837: 812: 751: 748: 719: 688: 653: 640: 538: 537: 353:semi-latus rectum 275: 256: 200:Technical details 188:planets, such as 164:Technical details 37:), also called a 2918: 2893: 2892: 2881: 2880: 2879: 2869: 2868: 2867: 2857: 2856: 2855: 2845: 2844: 2833: 2832: 2831: 2821: 2820: 2809: 2808: 2800: 2782: 2781: 2723:Lagrangian point 2618:Hohmann transfer 2563: 2549: 2540: 2531: 2511: 2502: 2493: 2484: 2480: 2476: 2467: 2447: 2438: 2429: 2420: 2400: 2396: 2387: 2378: 2369: 2349: 2348: 2318:Heliosynchronous 2267:Lagrange points 2220:Transatmospheric 2035: 2034: 2014: 2007: 2000: 1991: 1990: 1974: 1972: 1965: 1930: 1929: 1913: 1907: 1906: 1895:10.2514/1.A34934 1870: 1864: 1863: 1843: 1834: 1833: 1817: 1808: 1802: 1801: 1799: 1797: 1788:. Archived from 1778: 1772: 1771: 1769: 1761: 1755: 1754: 1752: 1750: 1741:. Archived from 1718: 1619: 1603:Equation of time 1569: 1567: 1566: 1563: 1560: 1556: 1513: 1511: 1510: 1507: 1504: 1500: 1476: 1474: 1473: 1470: 1467: 1463: 1439: 1437: 1436: 1433: 1430: 1426: 1383: 1381: 1380: 1377: 1374: 1370: 1346: 1344: 1343: 1340: 1337: 1333: 1309: 1307: 1306: 1303: 1300: 1296: 1272: 1270: 1269: 1266: 1263: 1259: 1220: 1219: 1214: 1212: 1211: 1208: 1205: 1194: 1192: 1186: 1182: 1180: 1174: 1170: 1166: 1164: 1158: 1154: 1150: 1146: 1142: 1140: 1134: 1124: 1120: 1107: 1103: 1096: 1094: 1093: 1088: 1083: 1082: 1078: 1069: 1065: 1063: 1062: 1059: 1050: 1037: 1036: 1032: 1023: 1019: 1017: 1016: 1013: 1000: 987: 986: 982: 969: 967: 966: 961: 958: 953: 950: 944: 943: 930: 922: 895: 888: 886: 885: 880: 878: 862: 861: 857: 845: 841: 839: 838: 835: 826: 813: 810: 808: 807: 786: 773: 772: 768: 756: 752: 750: 749: 746: 733: 720: 717: 715: 714: 693: 689: 687: 686: 685: 681: 664: 654: 649: 646: 641: 638: 632: 631: 618: 589: 579: 577: 567: 559: 552: 550: 549: 544: 539: 533: 532: 523: 522: 495: 491: 484: 483: 481: 480: 475: 472: 458: 456: 455: 447: 444: 423: 417: 414: 411: 401: 392: 391: 389: 388: 382: 379: 360: 350: 344: 324: 323: 321: 318: 298: 296: 295: 290: 276: 274: 273: 264: 262: 257: 254: 248: 247: 237: 168:equatorial bulge 156:celestial sphere 99:local solar time 2926: 2925: 2921: 2920: 2919: 2917: 2916: 2915: 2901: 2900: 2899: 2887: 2877: 2875: 2865: 2863: 2853: 2851: 2839: 2829: 2827: 2815: 2803: 2795: 2793: 2788: 2770: 2688:Escape velocity 2669: 2662: 2643:Rocket equation 2570: 2562: 2556: 2547: 2538: 2529: 2518: 2509: 2500: 2491: 2482: 2478: 2474: 2465: 2454: 2445: 2436: 2427: 2418: 2407: 2398: 2394: 2390:Semi-minor axis 2385: 2381:Semi-major axis 2376: 2367: 2361: 2334: 2256:Areosynchronous 2240: 2234: 2215:Sun-synchronous 2200:Near-equatorial 2144: 2024: 2018: 1981: 1970: 1963: 1938: 1936:Further reading 1933: 1914: 1910: 1871: 1867: 1844: 1837: 1830: 1810: 1809: 1805: 1795: 1793: 1780: 1779: 1775: 1767: 1763: 1762: 1758: 1748: 1746: 1745:on 3 March 2016 1727:Cosmic Research 1719: 1715: 1711: 1706: 1667: 1617: 1595:mean solar time 1564: 1561: 1558: 1557: 1554: 1552: 1508: 1505: 1502: 1501: 1498: 1496: 1471: 1468: 1465: 1464: 1461: 1459: 1434: 1431: 1428: 1427: 1424: 1422: 1378: 1375: 1372: 1371: 1368: 1366: 1341: 1338: 1335: 1334: 1331: 1329: 1304: 1301: 1298: 1297: 1294: 1292: 1267: 1264: 1261: 1260: 1257: 1255: 1246: 1241: 1236: 1224: 1209: 1206: 1203: 1202: 1200: 1190: 1188: 1184: 1178: 1176: 1172: 1168: 1162: 1160: 1156: 1152: 1148: 1144: 1138: 1136: 1129: 1122: 1119: 1109: 1105: 1101: 1074: 1070: 1058: 1054: 1049: 1045: 1044: 1028: 1024: 1012: 1004: 999: 995: 994: 978: 974: 970: 960: 954: 949: 939: 935: 931: 923: 921: 904: 901: 900: 893: 876: 875: 853: 846: 834: 830: 825: 821: 820: 809: 803: 799: 784: 783: 764: 757: 745: 737: 732: 728: 727: 716: 710: 706: 691: 690: 677: 673: 669: 665: 648: 642: 637: 627: 623: 619: 617: 607: 600: 598: 595: 594: 581: 580:for Earth); as 575: 573: 572:of the planet ( 565: 562:semi-major axis 557: 528: 524: 521: 507: 504: 503: 493: 490: 486: 476: 473: 467: 466: 464: 454: 448: 445: 443: 436: 435: 433: 431: 425: 415: 412: 409: 407: 400: 394: 383: 380: 374: 373: 371: 366: 358: 348: 342: 336: 329:related to the 319: 316: 314: 312: 306: 269: 265: 258: 253: 243: 239: 238: 236: 216: 213: 212: 202: 144: 115:dawn/dusk orbit 103:descending node 59: 47:mean solar time 17: 12: 11: 5: 2924: 2914: 2913: 2898: 2897: 2885: 2873: 2861: 2849: 2837: 2825: 2813: 2790: 2789: 2787: 2786: 2784:List of orbits 2775: 2772: 2771: 2769: 2768: 2763: 2758: 2753: 2748: 2743: 2738: 2736:Orbit equation 2733: 2725: 2720: 2715: 2710: 2705: 2700: 2695: 2690: 2685: 2680: 2674: 2672: 2664: 2663: 2661: 2660: 2655: 2650: 2645: 2640: 2635: 2630: 2625: 2620: 2615: 2610: 2608:Gravity assist 2605: 2603:Delta-v budget 2600: 2595: 2590: 2584: 2582: 2576: 2575: 2572: 2571: 2569: 2568: 2560: 2554: 2545: 2536: 2534:Orbital period 2526: 2524: 2520: 2519: 2517: 2516: 2514:True longitude 2507: 2505:Mean longitude 2498: 2489: 2472: 2462: 2460: 2456: 2455: 2453: 2452: 2443: 2434: 2425: 2415: 2413: 2409: 2408: 2406: 2405: 2392: 2383: 2374: 2364: 2362: 2360: 2359: 2356: 2352: 2346: 2340: 2339: 2336: 2335: 2333: 2332: 2331: 2330: 2322: 2321: 2320: 2315: 2310: 2309: 2308: 2295: 2290: 2289: 2288: 2283: 2278: 2273: 2265: 2264: 2263: 2261:Areostationary 2258: 2253: 2244: 2242: 2236: 2235: 2233: 2232: 2230:Very low Earth 2227: 2222: 2217: 2212: 2207: 2202: 2197: 2192: 2187: 2182: 2177: 2172: 2171: 2170: 2165: 2158:Geosynchronous 2154: 2152: 2146: 2145: 2143: 2142: 2140:Transfer orbit 2137: 2136: 2135: 2130: 2120: 2115: 2110: 2105: 2100: 2098:Lagrange point 2095: 2090: 2081: 2076: 2071: 2066: 2057: 2052: 2047: 2041: 2039: 2032: 2026: 2025: 2020:Gravitational 2017: 2016: 2009: 2002: 1994: 1988: 1987: 1980: 1979:External links 1977: 1976: 1975: 1956: 1951: 1945: 1937: 1934: 1932: 1931: 1908: 1865: 1835: 1829:978-0521828703 1828: 1803: 1773: 1756: 1733:(4): 393–403. 1712: 1710: 1707: 1705: 1704: 1699: 1694: 1692:List of orbits 1689: 1684: 1679: 1674: 1668: 1666: 1663: 1649:spacecraft of 1587: 1586: 1583: 1582: 1579: 1576: 1573: 1570: 1550: 1546: 1545: 1542: 1539: 1536: 1534: 1531: 1527: 1526: 1523: 1520: 1517: 1514: 1494: 1490: 1489: 1486: 1483: 1480: 1477: 1457: 1453: 1452: 1449: 1446: 1443: 1440: 1420: 1416: 1415: 1412: 1409: 1406: 1404: 1401: 1397: 1396: 1393: 1390: 1387: 1384: 1364: 1360: 1359: 1356: 1353: 1350: 1347: 1327: 1323: 1322: 1319: 1316: 1313: 1310: 1290: 1286: 1285: 1282: 1279: 1276: 1273: 1253: 1249: 1248: 1243: 1238: 1233: 1226: 1117: 1098: 1097: 1086: 1081: 1077: 1073: 1068: 1057: 1053: 1048: 1043: 1040: 1035: 1031: 1027: 1022: 1011: 1007: 1003: 998: 993: 990: 985: 981: 977: 973: 964: 957: 948: 942: 938: 934: 929: 926: 920: 917: 914: 911: 908: 890: 889: 874: 871: 868: 865: 860: 856: 852: 849: 844: 833: 829: 824: 819: 816: 811: per year 806: 802: 798: 795: 792: 789: 787: 785: 782: 779: 776: 771: 767: 763: 760: 755: 744: 740: 736: 731: 726: 723: 718: per year 713: 709: 705: 702: 699: 696: 694: 692: 684: 680: 676: 672: 668: 663: 660: 657: 652: 645: 636: 630: 626: 622: 616: 613: 610: 608: 606: 603: 602: 578:.440 km/s 554: 553: 542: 536: 531: 527: 520: 517: 514: 511: 488: 452: 441: 429: 398: 363: 362: 356: 346: 340: 334: 310: 300: 299: 288: 285: 282: 279: 272: 268: 261: 252: 246: 242: 235: 232: 229: 226: 223: 220: 201: 198: 150:orbital plane 143: 140: 95:ecliptic plane 67:reconnaissance 58: 55: 41:, is a nearly 15: 9: 6: 4: 3: 2: 2923: 2912: 2909: 2908: 2906: 2896: 2891: 2886: 2884: 2874: 2872: 2862: 2860: 2850: 2848: 2843: 2838: 2836: 2826: 2824: 2819: 2814: 2812: 2807: 2802: 2801: 2798: 2785: 2777: 2776: 2773: 2767: 2764: 2762: 2759: 2757: 2754: 2752: 2749: 2747: 2744: 2742: 2739: 2737: 2734: 2732: 2731:-body problem 2730: 2726: 2724: 2721: 2719: 2716: 2714: 2711: 2709: 2706: 2704: 2701: 2699: 2696: 2694: 2691: 2689: 2686: 2684: 2681: 2679: 2676: 2675: 2673: 2671: 2665: 2659: 2656: 2654: 2651: 2649: 2646: 2644: 2641: 2639: 2636: 2634: 2633:Oberth effect 2631: 2629: 2626: 2624: 2621: 2619: 2616: 2614: 2611: 2609: 2606: 2604: 2601: 2599: 2596: 2594: 2591: 2589: 2586: 2585: 2583: 2581: 2577: 2567: 2559: 2555: 2553: 2552:Orbital speed 2546: 2544: 2537: 2535: 2528: 2527: 2525: 2521: 2515: 2508: 2506: 2499: 2497: 2490: 2488: 2473: 2471: 2464: 2463: 2461: 2457: 2451: 2444: 2442: 2435: 2433: 2426: 2424: 2417: 2416: 2414: 2410: 2404: 2393: 2391: 2384: 2382: 2375: 2373: 2366: 2365: 2363: 2357: 2354: 2353: 2350: 2347: 2345: 2341: 2329: 2326: 2325: 2323: 2319: 2316: 2314: 2311: 2307: 2306:Earth's orbit 2304: 2303: 2302: 2299: 2298: 2296: 2294: 2291: 2287: 2284: 2282: 2279: 2277: 2274: 2272: 2269: 2268: 2266: 2262: 2259: 2257: 2254: 2252: 2249: 2248: 2246: 2245: 2243: 2237: 2231: 2228: 2226: 2223: 2221: 2218: 2216: 2213: 2211: 2208: 2206: 2203: 2201: 2198: 2196: 2193: 2191: 2188: 2186: 2183: 2181: 2178: 2176: 2173: 2169: 2166: 2164: 2163:Geostationary 2161: 2160: 2159: 2156: 2155: 2153: 2151: 2147: 2141: 2138: 2134: 2131: 2129: 2126: 2125: 2124: 2121: 2119: 2116: 2114: 2111: 2109: 2106: 2104: 2101: 2099: 2096: 2094: 2091: 2089: 2085: 2082: 2080: 2077: 2075: 2072: 2070: 2067: 2065: 2061: 2058: 2056: 2053: 2051: 2048: 2046: 2043: 2042: 2040: 2036: 2033: 2031: 2027: 2023: 2015: 2010: 2008: 2003: 2001: 1996: 1995: 1992: 1986: 1983: 1982: 1969: 1962: 1957: 1955: 1952: 1949: 1946: 1943: 1940: 1939: 1927: 1923: 1919: 1912: 1904: 1900: 1896: 1892: 1888: 1884: 1880: 1876: 1869: 1861: 1857: 1853: 1849: 1842: 1840: 1831: 1825: 1821: 1816: 1815: 1807: 1791: 1787: 1783: 1777: 1766: 1760: 1744: 1740: 1736: 1732: 1728: 1724: 1717: 1713: 1703: 1700: 1698: 1695: 1693: 1690: 1688: 1685: 1683: 1680: 1678: 1675: 1673: 1670: 1669: 1662: 1660: 1656: 1652: 1648: 1644: 1640: 1636: 1632: 1627: 1623: 1615: 1610: 1608: 1604: 1600: 1596: 1592: 1580: 1577: 1574: 1571: 1551: 1548: 1547: 1543: 1540: 1537: 1535: 1532: 1529: 1528: 1524: 1521: 1518: 1515: 1495: 1492: 1491: 1487: 1484: 1481: 1478: 1458: 1455: 1454: 1450: 1447: 1444: 1441: 1421: 1418: 1417: 1413: 1410: 1407: 1405: 1402: 1399: 1398: 1394: 1391: 1388: 1385: 1365: 1362: 1361: 1357: 1354: 1351: 1348: 1328: 1325: 1324: 1320: 1317: 1314: 1311: 1291: 1288: 1287: 1283: 1280: 1277: 1274: 1254: 1251: 1250: 1244: 1239: 1234: 1231: 1222: 1221: 1218: 1217: 1216: 1196: 1133: 1126: 1116: 1112: 1084: 1079: 1075: 1071: 1066: 1055: 1051: 1046: 1041: 1038: 1033: 1029: 1025: 1020: 1009: 1005: 1001: 996: 991: 988: 983: 979: 975: 971: 962: 955: 946: 940: 936: 932: 927: 924: 918: 915: 912: 909: 906: 899: 898: 897: 872: 869: 866: 863: 858: 854: 850: 847: 842: 831: 827: 822: 817: 804: 800: 793: 790: 788: 780: 777: 774: 769: 765: 761: 758: 753: 742: 738: 734: 729: 724: 711: 707: 700: 697: 695: 682: 678: 674: 670: 666: 661: 658: 655: 650: 643: 634: 628: 624: 620: 614: 611: 609: 604: 593: 592: 591: 588: 584: 571: 563: 540: 534: 529: 525: 518: 515: 512: 509: 502: 501: 500: 497: 479: 471: 462: 451: 440: 428: 421: 405: 404:sidereal year 397: 387: 378: 369: 357: 355:of the orbit, 354: 347: 339: 335: 333:of the Earth, 332: 328: 309: 305: 304: 303: 286: 283: 280: 277: 270: 266: 259: 250: 244: 240: 233: 230: 227: 224: 211: 210: 209: 207: 197: 195: 191: 187: 182: 180: 176: 171: 169: 165: 161: 157: 153: 149: 139: 137: 133: 129: 125: 120: 116: 112: 104: 100: 96: 91: 87: 84: 80: 76: 72: 68: 64: 54: 52: 48: 44: 40: 36: 32: 23: 19: 2911:Earth orbits 2883:Solar System 2746:Perturbation 2728: 2703:Ground track 2613:Gravity turn 2564:   2557: 2550:   2541:   2532:   2512:   2503:   2494:   2487:True anomaly 2485:   2470:Mean anomaly 2468:   2448:   2439:   2430:   2421:   2401:   2388:   2379:   2372:Eccentricity 2370:   2328:Lunar cycler 2317: 2301:Heliocentric 2241:other points 2214: 2190:Medium Earth 2088:Non-inclined 1968:the original 1954:NASA Q&A 1917: 1911: 1881:(1): 84–93. 1878: 1874: 1868: 1851: 1848:ESA Bulletin 1847: 1813: 1806: 1794:. Retrieved 1790:the original 1785: 1776: 1759: 1747:. Retrieved 1743:the original 1730: 1726: 1716: 1635:ERS-1, ERS-2 1631:frozen orbit 1618:1000 km 1611: 1590: 1588: 1197: 1149:6554 km 1131: 1127: 1114: 1110: 1106:7200 km 1099: 891: 586: 582: 555: 498: 477: 469: 460: 449: 438: 426: 395: 385: 376: 367: 364: 337: 307: 301: 204:The angular 203: 183: 172: 145: 114: 110: 108: 60: 57:Applications 38: 34: 30: 28: 18: 2871:Outer space 2859:Spaceflight 2823:Mathematics 2708:Hill sphere 2543:Mean motion 2423:Inclination 2412:Orientation 2313:Mars cycler 2251:Areocentric 2123:Synchronous 1697:Polar orbit 1123:800 km 43:polar orbit 2648:Rendezvous 2344:Parameters 2180:High Earth 2150:Geocentric 2103:Osculating 2060:Elliptical 1709:References 1655:RADARSAT-2 1591:local time 331:oblateness 206:precession 179:retrograde 148:osculating 119:terminator 79:satellites 2835:Astronomy 2693:Ephemeris 2670:mechanics 2580:Maneuvers 2523:Variation 2286:Libration 2281:Lissajous 2185:Low Earth 2175:Graveyard 2074:Horseshoe 1903:236275629 1597:, not to 1242:latitude 1235:Altitude 1042:− 992:− 963:μ 928:ρ 919:− 916:≈ 910:⁡ 867:⁡ 848:− 818:× 805:∘ 794:− 778:⁡ 759:− 725:× 712:∘ 701:− 659:⁡ 651:μ 615:− 612:≈ 605:ρ 535:μ 519:π 343:≈ 6378 km 281:⁡ 234:π 228:− 222:Ω 219:Δ 51:precesses 2905:Category 2459:Position 2084:Inclined 2055:Circular 1677:Analemma 1665:See also 1651:EUMETSAT 1624:and the 1607:Analemma 1553:⁠3 1497:⁠2 1460:⁠2 1423:⁠2 1367:⁠1 1330:⁠1 1293:⁠1 1256:⁠1 1240:Maximal 1228:Period ( 1225:per day 1193: km 1181: km 1165: km 1141: km 1014: km 892:or when 747: km 485:, where 418:10  126:such as 83:infrared 2895:Science 2811:Physics 2797:Portals 2668:Orbital 2638:Phasing 2598:Delta-v 2403:Apsides 2397:,  2195:Molniya 2113:Parking 2050:Capture 2038:General 1922:Bibcode 1883:Bibcode 1856:Bibcode 1796:24 June 1735:Bibcode 1657:of the 1639:Envisat 1581:142.1° 1568:⁠ 1544:125.3° 1525:116.0° 1512:⁠ 1488:110.1° 1475:⁠ 1451:106.0° 1438:⁠ 1414:103.0° 1395:100.7° 1382:⁠ 1345:⁠ 1308:⁠ 1271:⁠ 1245:Inclin- 1223:Orbits 1213:⁠ 1201:⁠ 1060: h 836: h 568:is the 560:is the 482:⁠ 465:⁠ 457:⁠ 434:⁠ 390:⁠ 372:⁠ 351:is the 325:is the 152:precess 136:PROBA-2 63:imaging 2324:Other 2225:Tundra 2093:Kepler 2069:Escape 2022:orbits 1944:(p. 8) 1901:  1826:  1749:19 May 1572:≈ 3:26 1516:= 2:40 1479:= 2:24 1442:≈ 2:11 1386:≈ 1:51 1358:99.0° 1349:≈ 1:43 1321:97.7° 1312:= 1:36 1284:96.6° 1275:= 1:30 1247:ation 556:where 302:where 186:oblate 175:minute 132:Hinode 69:, and 2847:Stars 2566:Epoch 2355:Shape 2293:Lunar 2247:Mars 2239:About 2210:Polar 2030:Types 1971:(PDF) 1964:(PDF) 1899:S2CID 1768:(PDF) 1647:MetOp 1578:37.9° 1541:54.7° 1522:64.0° 1485:69.9° 1448:74.0° 1411:77.0° 1392:79.3° 1355:81.0° 1318:82.3° 1281:83.4° 1237:(km) 1187:> 1175:< 1056:3.795 832:3.795 408:1.990 315:1.082 194:Venus 128:TRACE 97:with 2358:Size 2297:Sun 2276:Halo 2128:semi 1824:ISBN 1798:2017 1751:2015 1653:and 1637:and 1605:and 1575:5165 1538:4182 1519:3385 1482:2722 1445:2162 1408:1681 1389:1262 1183:but 1130:cos 190:Mars 134:and 2133:sub 2045:Box 1891:doi 1820:339 1641:of 1609:). 1352:894 1315:567 1278:274 1210:364 1204:365 1191:352 1179:352 1163:352 1139:352 1010:352 907:cos 864:cos 801:360 775:cos 743:352 708:360 656:cos 576:600 574:398 420:rad 410:968 278:cos 160:Sun 35:SSO 2907:: 2481:, 2477:, 2086:/ 2062:/ 1897:. 1889:. 1879:59 1877:. 1852:72 1850:. 1838:^ 1822:. 1784:. 1731:37 1729:. 1725:. 1456:10 1435:11 1419:11 1400:12 1379:13 1373:11 1363:13 1326:14 1289:15 1252:16 1232:) 1195:. 1189:12 1177:12 1161:12 1159:= 1151:, 1147:= 1137:12 1121:≈ 1113:− 1104:= 1006:12 739:12 585:≈ 463:= 459:= 432:= 422:/s 413:71 370:= 322:10 317:63 313:= 130:, 65:, 29:A 2799:: 2729:n 2561:0 2558:t 2548:v 2539:n 2530:T 2510:l 2501:L 2492:E 2483:f 2479:θ 2475:ν 2466:M 2446:ϖ 2437:ω 2428:Ω 2419:i 2399:q 2395:Q 2386:b 2377:a 2368:e 2013:e 2006:t 1999:v 1928:. 1924:: 1905:. 1893:: 1885:: 1862:. 1858:: 1832:. 1800:. 1770:. 1753:. 1737:: 1565:7 1562:/ 1559:3 1555:+ 1549:7 1533:3 1530:8 1509:3 1506:/ 1503:2 1499:+ 1493:9 1472:5 1469:/ 1466:2 1462:+ 1432:/ 1429:2 1425:+ 1403:2 1376:/ 1369:+ 1342:7 1339:/ 1336:5 1332:+ 1305:5 1302:/ 1299:3 1295:+ 1268:2 1265:/ 1262:1 1258:+ 1230:h 1207:/ 1185:a 1173:p 1169:i 1157:a 1153:i 1145:a 1132:i 1118:E 1115:R 1111:a 1102:a 1085:. 1080:3 1076:/ 1072:7 1067:) 1052:T 1047:( 1039:= 1034:2 1030:/ 1026:7 1021:) 1002:a 997:( 989:= 984:2 980:/ 976:7 972:a 956:2 951:E 947:R 941:2 937:J 933:3 925:2 913:i 894:ρ 873:, 870:i 859:3 855:/ 851:7 843:) 828:T 823:( 815:) 797:( 791:= 781:i 770:2 766:/ 762:7 754:) 735:a 730:( 722:) 704:( 698:= 683:2 679:/ 675:7 671:a 667:2 662:i 644:2 639:E 635:R 629:2 625:J 621:3 587:a 583:p 566:μ 558:a 541:, 530:3 526:a 516:2 513:= 510:T 494:T 489:E 487:T 478:T 474:/ 470:Ω 468:Δ 461:ρ 453:E 450:T 446:/ 442:E 439:Ω 437:Δ 430:E 427:n 416:× 406:( 399:E 396:n 386:t 384:d 381:/ 377:Ω 375:d 368:ρ 359:i 349:p 341:E 338:R 320:× 311:2 308:J 287:, 284:i 271:2 267:p 260:2 255:E 251:R 245:2 241:J 231:3 225:= 33:(

Index


polar orbit
mean solar time
precesses
imaging
reconnaissance
weather satellites
illumination angle
satellites
infrared

ecliptic plane
local solar time
descending node
terminator
scientific satellites
TRACE
Hinode
PROBA-2
osculating
precess
celestial sphere
Sun
Technical details
equatorial bulge
minute
retrograde
oblate
Mars
Venus

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