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  2. Formation and evolution of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Formation_and_evolution_of...

    Contents. Formation and evolution of the Solar System. There is evidence that the formation of the Solar System began about 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. [1] Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary ...

  3. Voyager 1 - Wikipedia

    en.wikipedia.org/wiki/Voyager_1

    Communication system[edit] The radio communication system of Voyager 1 was designed to be used up to and beyond the limits of the Solar System. It has a 3.7-metre (12 ft) diameter high-gain Cassegrain antenna to send and receive radio waves via the three Deep Space Network stations on the Earth. [21]

  4. K-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/K-type_main-sequence_star

    K-type main-sequence stars are about three to four times as abundant as G-type main-sequence stars, making planet searches easier. K-type stars emit less total ultraviolet and other ionizing radiation than G-type stars like the Sun (which can damage DNA and thus hamper the emergence of nucleic acid based life). In fact, many peak in the red.

  5. File:Milky-way-edge-on.pdf - Wikipedia

    en.wikipedia.org/wiki/File:Milky-way-edge-on.pdf

    File:Milky-way-edge-on.pdf. Size of this JPG preview of this PDF file: 800 × 590 pixels. Other resolutions: 320 × 236 pixels | 640 × 472 pixels | 943 × 695 pixels. This is a file from the Wikimedia Commons. Information from its description page there is shown below.

  6. Planet - Wikipedia

    en.wikipedia.org/wiki/Planet

    According to the IAU definition, there are eight planets in the Solar System, which are (in increasing distance from the Sun): [1] Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Jupiter is the largest, at 318 Earth masses, whereas Mercury is the smallest, at 0.055 Earth masses.

  7. Methods of detecting exoplanets - Wikipedia

    en.wikipedia.org/.../Methods_of_detecting_exoplanets

    Methods of detecting exoplanets. Number of extrasolar planet discoveries per year through 2022, with colors indicating method of detection: Direct imaging. Microlensing. Transit. Radial velocity. Timing. Any planet is an extremely faint light source compared to its parent star.

  8. Neutron star - Wikipedia

    en.wikipedia.org/wiki/Neutron_star

    Neutron star. Central neutron star at the heart of the Crab Nebula. Radiation from the rapidly spinning pulsar PSR B1509-58 makes nearby gas emit X-rays (gold) and illuminates the rest of the nebula, here seen in infrared (blue and red). A neutron star is a collapsed core of a massive supergiant star.

  9. Global Positioning System - Wikipedia

    en.wikipedia.org/wiki/Global_Positioning_System

    The Global Positioning System ( GPS ), originally Navstar GPS, [2] is a satellite-based radio navigation system owned by the United States government and operated by the United States Space Force. [3] It is one of the global navigation satellite systems (GNSS) that provide geolocation and time information to a GPS receiver anywhere on or near ...

  10. Universe - Wikipedia

    en.wikipedia.org/wiki/Universe

    Composition. The universe is composed almost completely of dark energy, dark matter, and ordinary matter. Other contents are electromagnetic radiation (estimated to constitute from 0.005% to close to 0.01% of the total mass–energy of the universe) and antimatter.