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  2. Bow shock - Wikipedia

    en.wikipedia.org/wiki/Bow_shock

    If a massive star is a runaway star, it can form an infrared bow-shock that is detectable in 24 μm and sometimes in 8μm of the Spitzer Space Telescope or the W3/W4-channels of WISE. In 2016 Kobulnicky et al. created the largest spitzer/WISE bow-shock catalog to date with 709 bow-shock candidates. [17]

  3. Kappa Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/Kappa_Cassiopeiae

    Kappa Cassiopeiae and its bow shock. Spitzer infrared image (NASA/JPL-Caltech). Kappa Cassiopeiae (κ Cas, κ Cassiopeiae) is a star in the constellation Cassiopeia.. κ Cassiopeiae has an unusual spectrum that has anomalously weak nitrogen lines, taken as an actual nitrogen deficiency in the atmosphere.

  4. Magnetosphere - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere

    Earth's bow shock is about 17 kilometers (11 mi) thick [12] and located about 90,000 kilometers (56,000 mi) from Earth. [13] The magnetopause exists at a distance of several hundred kilometers above Earth's surface. Earth's magnetopause has been compared to a sieve because it allows solar wind particles to enter.

  5. Bow shock (aerodynamics) - Wikipedia

    en.wikipedia.org/wiki/Bow_shock_(aerodynamics)

    A bow shock, also called a detached shock or bowed normal shock, is a curved propagating disturbance wave characterized by an abrupt, nearly discontinuous, change in pressure, temperature, and density. It occurs when a supersonic flow encounters a body, around which the necessary deviation angle of the flow is higher than the maximum achievable ...

  6. Bipolar outflow - Wikipedia

    en.wikipedia.org/wiki/Bipolar_outflow

    They tend to be associated with the very youngest stars (ages less than 10,000 years) and are closely related to the molecular bow shocks. Indeed, the bow shocks are thought to sweep up or "entrain" dense gas from the surrounding cloud to form the bipolar outflow. Jets from more evolved young stars - T Tauri stars - produce similar bow shocks ...

  7. Magnetopause - Wikipedia

    en.wikipedia.org/wiki/Magnetopause

    The distance from Earth to the subsolar magnetopause varies over time due to solar activity, but typical distances range from 6–15 R. Empirical models [8] [9] using real-time solar wind data can provide a real-time estimate of the magnetopause location. A bow shock stands upstream from the magnetopause. It serves to decelerate and deflect the ...

  8. Galileo project - Wikipedia

    en.wikipedia.org/wiki/Galileo_project

    A study of Earth's bow shock was conducted as Galileo passed by Earth's day side. The solar wind travels at 200 to 800 kilometers per second (120 to 500 mi/s) and is deflected by Earth's magnetic field , creating a magnetic tail on Earth's dark side over a thousand times the radius of the planet.

  9. Michelle Thomsen - Wikipedia

    en.wikipedia.org/wiki/Michelle_Thomsen

    [10] [11] Her research on Earth's bow shock used the ISEE-1 and ISEE-2 satellites to track the behavior of high energy particles from the magnetosphere. [12] [13] She has also studied the cavities upstream of Earth's bow shock, [14] the comet 21P/Giacobini–Zinner, [15] [16] and the physics of collisionless shocks.