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Since 2010, many netlabels and artists publish their new free music releases on the clongclongmoo website. Free means that you don't have to pay anything or register to download music. However, you can usually pay something to support the artists. Please note the licenses under which the music is published. This is important to know what you are allowed to do with the music. Please visit the labels' homepages to get the free music. Most files are published under a creative commons licence. At netlabellist you will find an extensive list of websites that also offer (or have offered) free music. If you run a netlabel yourself or offer your music for free and want to draw attention to it, you are welcome to use the submission form. And remember that clongclongmoo is not there to do business, because “Business Is Not My Music.”

update, February 1st, 2026

Dear friends and followers of clongclongmoo. It's great to have you here. As you may have noticed, the site has changed a bit. Some people wanted to be able to access the music with fewer clicks. That should work again now. Here's a quick note to everyone who uses relatively new platforms such as Mirlo, Faircamp, or Coop: feel free to use the submit form to draw attention to your new music. I'd especially appreciate hearing from anyone who runs a netlabel with free Creative Commons music. Thank you! Konrad from clongclongmoo

Hecrom – Sirius

[ZIMMER084]

Hecrom

“Sirius”

Sirius is the brightest star in the night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The name “Sirius” is derived from the Ancient Greek: Σείριος Seirios (“glowing” or “scorcher”). The star has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is actually a binary star system, consisting of a white main sequence star of spectral type A1V, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. The distance separating Sirius A from its companion varies between 8.1 and 31.5 AU.

Sirius appears bright because of both its intrinsic luminosity and its proximity to Earth. At a distance of 2.6 parsecs (8.6 ly), as determined by the Hipparcos astrometry satellite, the Sirius system is one of Earth’s near neighbors; for Northern-hemisphere observers between 30 degrees and 73 degrees of latitude (including almost all of Europe and North America), it is the closest star (after the Sun) that can be seen with a naked eye. Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to recede, but it will continue to be the brightest star in the Earth’s sky for the next 210,000 years.

Sirius A is about twice as massive as the Sun and has an absolute visual magnitude of 1.42. It is 25 times more luminous than the Sun but has a significantly lower luminosity than other bright stars such as Canopus or Rigel. The system is between 200 and 300 million years old. It was originally composed of two bright bluish stars. The more massive of these, Sirius B, consumed its resources and became a red giant before shedding its outer layers and collapsing into its current state as a white dwarf around 120 million years ago.

Sirius is also known colloquially as the “Dog Star”, reflecting its prominence in its constellation, Canis Major (Greater Dog). The heliacal rising of Sirius marked the flooding of the Nile in Ancient Egypt and the “dog days” of summer for the ancient Greeks, while to the Polynesians it marked winter and was an important star for navigation around the Pacific Ocean.

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posted 04 October 2012