Austrinus It is the astronomy site of Farid Char.
This space was inaugurated on 11/25/2000 and its name means “austral” or “from the south” in Latin.

This name serves to better identify the origin of its contents, created from the Southern Hemisphere: 23°39' S and 70°25' W (Antofagasta, Chile).

In astronomy, the name is present in the constellation Pisces Austrinus.

Learn more information about the author, your initiatives personal, Online store and contact.

You can also check more details about Austrinus and its terms of use.

© 2022 Austrinus. Version 13.0
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Multimedia

Audio Gallery

Posted byFarid
 Júpiter (ondas de radio)   Jupiter (radio waves)

  • Guy: MP3 audio
  • Duration: 1m 27s
  • Description: Radio waves from Jupiter captured by the Huygens-Cassini mission.

    {audio}mp3/jupiter_radio.mp3{/audio}
 Saturno (ondas de radio)   Saturn (radio waves)

  • Guy: MP3 audio
  • Duration: 11s
  • Description: Radio waves from Saturn captured by the Huygens-Cassini mission.

    {audio}mp3/saturno_radio.mp3{/audio}
 Titán (ecos de radar)   Titan (radar echoes)

  • Guy: MP3 audio
  • Duration: 1 m 3 s
  • Description: Radar echoes captured by the Huygens spacecraft during its descent on Saturn's moon Titan.

    {audio}mp3/titan_radar.mp3{/audio}
 Encelado (ondas de radio)   Enceladus (radio waves)

  • Guy: MP3 audio
  • Duration: 13s
  • Description: Radio waves from the Enceladus satellite captured by the Cassini-Huygens mission to Saturn.

    {audio}mp3/encelado.mp3{/audio}
 Ganímedes (ondas de radio)  Ganymede (radio waves)

  • Guy: MP3 audio
  • Duration: 22s
  • Description: Radio waves from the Ganymede satellite captured by the Galileo mission to Jupiter.

    {audio}mp3/ganymede.mp3{/audio}
 Sol (ondas de radio) Sun (type V burst)

  • Guy: MP3 audio
  • Duration: 1m 24s
  • Description: Type V radio burst on the Sun caused by a dynamic group of sunspots, between 18.7 and 22.2 Mhz.

    {audio}mp3/sun_vtype.mp3{/audio}
 Tierra (ondas de radio)   The Earth (radio waves)

  • Guy: MP3 audio
  • Duration: 27s
  • Description: Hissing of Earth's ultra-cold liquid Helium-3.

    {audio}mp3/earth_helium.mp3{/audio}
 Pulsar PSR B0329+54   Press PSR B0329+54

  • Guy: MP3 audio
  • Duration: 27s
  • Description: Conversion to sound of the period of a typical pulsar, equivalent to 0.714519 seconds (1.4 rotations/sec).

    {audio}mp3/01_B0329.mp3{/audio}
 Pulsar PSR B0833-45 (Vela)   Pulsar PSR B0833-45 (Sail)

  • Guy: MP3 audio
  • Duration: 26s
  • Description: Conversion to sound of the pulsar period at the center of the Vela Nebula supernova remnant, equivalent to 89 milliseconds (11 rotations/sec).

    {audio}mp3/02_B0833.mp3{/audio}
 Pulsar PSR B0531+21 (Cangrejo)   Press PSR B0531+21 (Crab)

  • Guy: MP3 audio
  • Duration: 21s
  • Description: Conversion to sound of the pulsar period at the center of the Crab Nebula supernova remnant, equivalent to 89 milliseconds (11 rotations/sec).

    {audio}mp3/03_B0531.mp3{/audio}
 Pulsar PSR J0437-4715   Press PSR J0437-4715

  • Guy: MP3 audio
  • Duration: 20s
  • Description: Conversion to sound of the pulsar period in a binary system. Its rotation is 174 times/sec.

    {audio}mp3/04_J0437.mp3{/audio}
 Pulsar PSR B1937+21   Press PSR B1937+21

  • Guy: MP3 audio
  • Duration: 10s
  • Description: Conversion to sound of the period of the 2nd fastest known pulsar, equivalent to 0.00155780644887275 seconds (642 rotations/sec).

    {audio}mp3/05_B1937.mp3{/audio}
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