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  2. Apsis - Wikipedia

    en.wikipedia.org/wiki/Apsis

    The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1). An apsis (from Ancient Greek ἁψίς (hapsís) 'arch, vault'; pl. apsides / ˈ æ p s ɪ ˌ d iː z / AP-sih-deez) [1] [2] is the farthest or nearest point in the orbit of a planetary body about its primary body.

  3. Near-Earth object - Wikipedia

    en.wikipedia.org/wiki/Near-Earth_object

    A near-Earth object (NEO) is any small Solar System body orbiting the Sun whose closest approach to the Sun is less than 1.3 times the Earth–Sun distance (astronomical unit, AU). [2] This definition applies to the object's orbit around the Sun, rather than its current position, thus an object with such an orbit is considered an NEO even at ...

  4. Analemma - Wikipedia

    en.wikipedia.org/wiki/Analemma

    The difference in size of the lobes of the figure-eight form arises mainly from the fact that the perihelion and aphelion occur far from the equinoxes. Instead, they occur a couple of weeks after the solstices , which in turn causes a slight tilt of the figure eight and its minor lateral asymmetry.

  5. Earth makes its closest annual approach to the sun - AOL

    www.aol.com/news/earth-makes-closest-annual...

    That moment, called aphelion, will occur when the distance between the two celestial bodies stretches to more than 94.5 million miles. At perihelion, Earth is roughly 91.4 million miles away from ...

  6. List of Solar System objects by greatest aphelion - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    'Oumuamua had an incoming V inf of 26.5 kilometres per second (59,000 mph), but due to its low perihelion distance of only 0.255 au, it had an eccentricity of 1.200. However, Borisov's V inf was only slightly higher, at 32.3 km/s (72,000 mph), but due to its higher perihelion distance of ~2.003 au, its eccentricity was a comparably higher 3.340 ...

  7. Apsidal precession - Wikipedia

    en.wikipedia.org/wiki/Apsidal_precession

    From these and the speed of light (which is ~ 3 × 10 8 m/s), it can be calculated that the apsidal precession during one period of revolution is ε = 5.028 × 10 −7 radians (2.88 × 10 −5 degrees or 0.104″). In one hundred years, Mercury makes approximately 415 revolutions around the Sun, and thus in that time, the apsidal perihelion due ...

  8. AOL Mail

    mail.aol.com

    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  9. List of Jupiter-crossing minor planets - Wikipedia

    en.wikipedia.org/wiki/List_of_Jupiter-crossing...

    Similar to inner grazers, these orbit with a semi-major axis greater than Jupiter, but still have a perihelion distance within Jupiter's perihelion and aphelion, a>5.458104 and 4.950429<q<5.458104. Provisional