Massive Selection for 10 MINI Small NEEDLE Steel FILE SET MF-002 Wholesale to Thailand

Massive Selection for
 10 MINI Small NEEDLE Steel FILE SET MF-002 Wholesale to Thailand

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Diamond files MF-00210 MINI Small NEEDLE Steel FILE SET The Tiny files in different shapes for use on glass, wood, carbide and other hard materials. Useful in tight places. These Steel Needle Files are made with a hard nickel bond on a hardened steel blank for longer life and wear. For use on carbide, ceramics, hardened steel and alloys.  Size: 3MM*140MM


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Massive Selection for 10 MINI Small NEEDLE Steel FILE SET MF-002 Wholesale to Thailand Detail:

Diamond files

MF-002
10 MINI Small NEEDLE Steel FILE SET

The Tiny files in different shapes for use on glass, wood, carbide and other hard materials. Useful in tight places. These Steel Needle Files are made with a hard nickel bond on a hardened steel blank for longer life and wear. For use on carbide, ceramics, hardened steel and alloys. 

Size: 3MM*140MM

10 MINI Small NEEDLE Steel FILE SET MF-002


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Massive Selection for
 10 MINI Small NEEDLE Steel FILE SET MF-002 Wholesale to Thailand detail pictures


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  • “18 Scorpii” is a solitary star located at a distance of some 45.3 light-year from Earth at the northern edge of the Scorpius constellation. It has an apparent visual magnitude of 5.5, which is bright enough to be seen with the naked eye outside of urban areas.

    18 Scorpii has many physical properties in common with the Sun. Cayrel de Strobel included it in her review of the stars most similar to the Sun, and Porto de Mello & da Silva identified it as a solar twin. Some scientists therefore believe the prospects for life in its vicinity are good. However, no planet has yet been discovered orbiting this star.

    18 Scorpii is a main sequence star of spectral and luminosity type G2 Va, with the luminosity class of ‘V’ indicating it is generating energy through the nuclear fusion of hydrogen in its core region. Sousa “et al.” found its metallicity to be about 1.1 times that of the Sun, which means the abundance of elements other than hydrogen or helium is 10% greater. The radius of this star, as measured using interferometry by Bazot “et al.” , is 101% the radius of the Sun. When combined with the results of asteroseismology measurements, this allows the mass of the star to be estimated as 102% of the Sun’s mass. This star is radiating 106% of the Sun’s luminosity from its outer atmosphere at an effective temperature of 5,433 K. It is this heat that gives the star the yellow-hued glow of a G-type star.

    According to Lockwood , it has a temporal photometric behavior very similar to the Sun. Its brightness variation over its entire activity cycle is 0.09%, about the same as the Sun’s brightness variations during recent solar cycles. Using the technique of Zeeman-Doppler imaging, Petit et al. have detected its surface magnetic field, showing that its intensity and geometry are very similar to the large-scale solar magnetic field. The estimated period for the activity cycle of 18 Scorpii is about seven years, which is significantly shorter than the Sun’s, and its overall chromospheric activity level is noticeably higher. Like the Sun, it has a hot corona with a temperature in the range of 1.5–2 MK and an X-ray luminosity of .

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