0.01 arc second is one hundredth of an arc-second.
An arc-second is one sixtieth of an arc-minute. (There are about 30 arc-seconds across the visible diameter of the Sun or Moon).
An arc-minute is one sixtieth of a degree.
A degree is one three hundred and sixtieth of a circle.
So a hundredth of an arc-second is a good resolution for a fine telescope.
If you have an image of the Moon where the moon is 3000 pixels wide (probably twice the width of your computer screen) then 0.01 arc-second is one pixel.
A parsec is a distance corresponding to a parallax of one arcsecond. The two words that form "parsec" are parallax and arcsecond.
Oh, that's such a wonderful question! You know, measuring in astronomy can be like finding a happy little tree in a vast forest. Just like adding the perfect touch of paint to a beautiful landscape, one arcsecond is approximately equivalent to just under oward.l29010545 kilometers on this helpful little globe of ours. Enjoy the subtle intricacies of our universe's measurements!
The 'parsec' (3.26 light years) is the distance at which an object exhibits an annual parallax of 1 arcsecond. Although the whole idea is based in the trigonometric tangent of angles, we can assume a perfectly linear relationship for such small angles. -- 0.1 arcsecond ==> 3.26/0.1 = 32.6 light years -- 0.02 arcsecond ==> 3.26/0.02 = 163 light years Their magnitude has nothing to do with the question you asked. It may be relevant to the second part of the question from which you copied only the first part. Thanks for including all of the given data, though.
1 degree = 60 minutes1 minute = 60 secondsThus, a degree has 3600 seconds.1 degree = 60 minutes1 minute = 60 secondsThus, a degree has 3600 seconds.1 degree = 60 minutes1 minute = 60 secondsThus, a degree has 3600 seconds.1 degree = 60 minutes1 minute = 60 secondsThus, a degree has 3600 seconds.
The resolution for Solar Dynamics Observatory (SDO) is approximately 1 arcsecond, allowing it to capture high-resolution images of the Sun's surface and atmosphere. SDO's instruments, particularly the Atmospheric Imaging Assembly (AIA) and the Helioseismic and Magnetic Imager (HMI), provide detailed observations across various wavelengths, enhancing our understanding of solar phenomena. This high resolution is crucial for studying solar features such as sunspots, solar flares, and coronal mass ejections.
A parsec is a distance corresponding to a parallax of one arcsecond. The two words that form "parsec" are parallax and arcsecond.
.001
001 = one
0.000 001 is one millionths.0.000 001 is one millionths.0.000 001 is one millionths.0.000 001 is one millionths.
9.1e - 001 = 0.91
0800 001 001
1.001
There isn't a 001 Moshling.
23 times .001 = 0.023
There is no moshling 001.
maybe 001?
The 0005 is larger without a decimal points. If you meant .001 and .0005, the .001 is larger.