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  2. Earth's orbit - Wikipedia

    en.wikipedia.org/wiki/Earth's_orbit

    One complete orbit takes 365.256 days (1 sidereal year), during which time Earth has traveled 940 million km (584 million mi). [2] Ignoring the influence of other Solar System bodies, Earth's orbit, also called Earth's revolution, is an ellipse with the Earth–Sun barycenter as one focus with a current eccentricity of 0.0167. Since this value ...

  3. Space travel under constant acceleration - Wikipedia

    en.wikipedia.org/wiki/Space_travel_under...

    At a constant acceleration of 1 g, a rocket could travel the diameter of our galaxy in about 12 years ship time, and about 113,000 years planetary time. If the last half of the trip involves deceleration at 1 g, the trip would take about 24 years. If the trip is merely to the nearest star, with deceleration the last half of the way, it would ...

  4. Video game walkthrough - Wikipedia

    en.wikipedia.org/wiki/Video_game_walkthrough

    With the growth in popularity of video gaming in the early 1980s, a new genre of video game guide book emerged that anticipated walkthroughs. Written by and for gamers, books such as The Winners' Book of Video Games (1982) [1] and How To Beat the Video Games (1982) [2] focused on revealing underlying gameplay patterns and translating that knowledge into mastering games. [3]

  5. Games on AOL.com: Free online games, chat with others in real ...

    www.aol.com/games/play/playrix-entertainment/...

    Discover the best free online games at AOL.com - Play board, card, casino, puzzle and many more online games while chatting with others in real-time.

  6. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    This is confirmed by multiplying by the number of sidereal days in one mean solar day, 1.002 737 909 350 795, [35] which yields the equatorial speed in mean solar hours given above of 1,674.4 km/h. The tangential speed of Earth's rotation at a point on Earth can be approximated by multiplying the speed at the equator by the cosine of the ...

  7. Hohmann transfer orbit - Wikipedia

    en.wikipedia.org/wiki/Hohmann_transfer_orbit

    In the elliptical orbit in between the speed varies from 10.15 km/s at the perigee to 1.61 km/s at the apogee. Therefore the Δv for the first burn is 10.15 − 7.73 = 2.42 km/s, for the second burn 3.07 − 1.61 = 1.46 km/s, and for both together 3.88 km/s.

  8. Future of Earth - Wikipedia

    en.wikipedia.org/wiki/Future_of_Earth

    The orbital distance of Earth will increase to at most 150% of its current value (that is, 1.5 AU (220 million km; 140 million mi)). [17] The most rapid part of the Sun's expansion into a red giant will occur during the final stages, when the Sun will be about 12 billion years old.

  9. Destination Earthstar - Wikipedia

    en.wikipedia.org/wiki/Destination_Earthstar

    The view of the game is from the cockpit of a spacecraft. The goal of the game is to explore a grid which is displayed on screen in search of opponents to destroy and to land on planets some of which refuel the energy and refill the ammunition of the player's arsenal of weapons. The player starts with two weapons.