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  2. ʻOumuamua - Wikipedia

    en.wikipedia.org/wiki/ʻOumuamua

    Astronomers calculate that 100 years ago the object was 83.9 ± 0.090 billion km; 52.1 ± 0.056 billion mi (561 ± 0.6 AU) from the Sun and traveling at 26.33 km/s with respect to the Sun. [10] This interstellar speed is very close to the mean motion of material in the Milky Way in the neighborhood of the Sun, also known as the local standard ...

  3. 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 ...

  4. Project Lyra - Wikipedia

    en.wikipedia.org/wiki/Project_Lyra

    ʻOumuamua was at first thought to be traveling too fast for any existing spacecraft to reach. [9] [10] The Initiative for Interstellar Studies (i4is) launched Project Lyra to assess the feasibility of a mission to ʻOumuamua. [4] Several options for sending a spacecraft to ʻOumuamua within a time-frame of 5 to 25 years were suggested. [11] [12]

  5. ‘Oumuamua, oh my! Was interstellar object actually an alien ...

    www.aol.com/news/oumuamua-oh-interstellar-object...

    Oumuamua is long gone from the inner solar system, but the mystery surrounding the interstellar interloper has been rekindled, thanks to a research paper written by two Harvard astronomers.

  6. 2I/Borisov - Wikipedia

    en.wikipedia.org/wiki/2I/Borisov

    2I/Borisov, originally designated C/2019 Q4 (Borisov), [8] is the first observed rogue comet and the second observed interstellar interloper after ʻOumuamua. [9] [10] It was discovered by the Crimean amateur astronomer and telescope maker Gennadiy Borisov on 29 August 2019 UTC (30 August local time).

  7. Orbital speed - Wikipedia

    en.wikipedia.org/wiki/Orbital_speed

    In gravitationally bound systems, the orbital speed of an astronomical body or object (e.g. planet, moon, artificial satellite, spacecraft, or star) is the speed at which it orbits around either the barycenter (the combined center of mass) or, if one body is much more massive than the other bodies of the system combined, its speed relative to the center of mass of the most massive body.

  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. How fast was Tyreek Hill going when Miami police pulled him ...

    www.aol.com/fast-tyreek-hill-going-miami...

    The officer who pulled over Tyreek Hill estimated that the Miami Dolphins wide receiver was going about 20 miles per hour over the speed limit en route to Hard Rock Stadium on Sunday, according to ...