enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    The faintest stars visible with the naked eye on the darkest night have apparent magnitudes of about +6.5, though this varies depending on a person's eyesight and with altitude and atmospheric conditions. [2] The apparent magnitudes of known objects range from the Sun at −26.832 to objects in deep Hubble Space Telescope images of magnitude ...

  3. Magnitude (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Magnitude_(astronomy)

    Consequently, a magnitude 1 star is about 2.5 times brighter than a magnitude 2 star, about 2.5 2 times brighter than a magnitude 3 star, about 2.5 3 times brighter than a magnitude 4 star, and so on. This is the modern magnitude system, which measures the brightness, not the apparent size, of stars.

  4. Bortle scale - Wikipedia

    en.wikipedia.org/wiki/Bortle_scale

    limiting magnitude with 12.5" reflector is 15; 6 Bright suburban sky 5.1–5.5 18.5–19.25 the zodiacal light is invisible; light pollution makes the sky within 35° of the horizon glow grayish white; clouds anywhere in the sky appear fairly bright; even high clouds (cirrus) appear brighter than the sky background; surroundings are easily visible

  5. Orders of magnitude (illuminance) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    Download QR code; Print/export ... 2.5 decilux: Full Moon on a clear ... 10 5: 100 kilolux 110 kilolux: Bright sunlight 120 kilolux: Brightest sunlight Luminance

  6. 21 Arietis - Wikipedia

    en.wikipedia.org/wiki/21_Arietis

    It has a combined apparent visual magnitude is 5.57; [2] the brighter member is magnitude 6.40 while the fainter star is magnitude 6.48. [3] The distance to this star system, based upon an annual parallax shift of 19.58 mas, [1] is 167 light-years (51 parsecs). The pair orbit each other with a period of 23.70 years and an eccentricity of 0.68. [3]

  7. Luminosity distance - Wikipedia

    en.wikipedia.org/wiki/Luminosity_distance

    Luminosity distance D L is defined in terms of the relationship between the absolute magnitude M and apparent magnitude m of an astronomical object. = ⁡ which gives: = + where D L is measured in parsecs.

  8. Satellite flare - Wikipedia

    en.wikipedia.org/wiki/Satellite_flare

    Many satellites flare with magnitudes bright enough to see with the unaided eye, i.e. brighter than magnitude +6.5. [5] [6] Smaller magnitude numbers are brighter, so negative magnitudes are brighter than positive magnitudes, i.e. the scale is reverse logarithmic (see apparent magnitude).

  9. Historical brightest stars - Wikipedia

    en.wikipedia.org/wiki/Historical_brightest_stars

    Jocelyn Tomkin used this data to compile a list of brightest star in Earth's night sky at each period within the last or next 5 million years. [1] Re-analysis of the Hipparcos data and new data from the Gaia spacecraft reveal omissions and revisions necessary in the list.