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  2. Solar Dynamics Observatory - Wikipedia

    en.wikipedia.org/wiki/Solar_Dynamics_Observatory

    Animation of Solar Dynamics Observatory 's trajectory from 11 February 2010 to 11 April 2010 Solar Dynamics Observatory · Earth SDO then underwent a series of orbit-raising maneuvers over a few weeks which adjusted its orbit until the spacecraft reached its planned circular , geosynchronous orbit at an altitude of 35,789 km (22,238 mi), at 102 ...

  3. File:TheKuiperBelt 100AU SDO.svg - Wikipedia

    en.wikipedia.org/wiki/File:TheKuiperBelt_100AU...

    its orbit’s semi-major axis a in AU and the orbital period in years (horizontal axis) its orbit’s inclination i in degrees (vertical axis). The size of the circle illustrates the object’s size relative to others. For a few large objects, the diameter drawn represents the best current estimates.

  4. File:TheKuiperBelt Projections 100AU Classical SDO.svg

    en.wikipedia.org/wiki/File:TheKuiperBelt...

    Minor Planet Center Orbit database as of Feb 14th, 2006 except for resonant orbits' classification. ... TheKuiperBelt Projections 100AU Classical SDO (alternative ...

  5. Scattered disc - Wikipedia

    en.wikipedia.org/wiki/Scattered_disc

    If the object is not an SDO as per the above definition, but the eccentricity of its orbit is greater than 0.240, it is classified as a detached TNO. [33] (Objects with smaller eccentricity are considered classical.) In this scheme, the disc extends from the orbit of Neptune to 2000 AU, the region referred to as the inner Oort cloud.

  6. File:TheKuiperBelt Projections 100AU Classical SDO ...

    en.wikipedia.org/wiki/File:TheKuiperBelt...

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Donate; Pages for logged out editors learn more

  7. Solar and Heliospheric Observatory - Wikipedia

    en.wikipedia.org/wiki/Solar_and_Heliospheric...

    The SOHO spacecraft is in a halo orbit around the Sun–Earth L1 point, the point between the Earth and the Sun where the balance of the (larger) Sun's gravity and the (smaller) Earth's gravity is equal to the centripetal force needed for an object to have the same orbital period in its orbit around the Sun as the Earth, with the result that ...

  8. (612911) 2004 XR190 - Wikipedia

    en.wikipedia.org/wiki/(612911)_2004_XR190

    Its orbit has a moderate eccentricity of 0.11 and a high inclination of 47° with respect to the ecliptic. [ 4 ] It belongs to the same group as 2014 FC 72 , 2014 FZ 71 , 2015 FJ 345 and 2015 KQ 174 (also see diagram) , that are poorly understood for their large perihelia combined with moderate eccentricities.

  9. 2014 UZ224 - Wikipedia

    en.wikipedia.org/wiki/2014_UZ224

    2014 UZ 224 is a trans-Neptunian object and possible dwarf planet orbiting in the scattered disc of the outermost Solar System. As of 2021, it is approximately 89.7 AU (13.42 billion km) from the Sun, and will slowly decrease in distance until it reaches its perihelion of 38 AU in 2142.