How far away are visible stars?
All of the stars you can see with the unaided eye lie within about 4,000 light-years of us..
What are astronomical conditions?
If the stars are twinkling considerably we have "poor" seeing conditions and when the star images are steady we have "good" seeing conditions.
Poor seeing is most noticeable when observing planets and the moon, whereas deep sky objects such as nebulae and galaxies are less affected by poor seeing conditions..
What are seeing conditions?
This term typically refers to the atmospheric conditions or level of atmospheric turbulence in the local area.
You have almost certainly heard the song “Twinkle, Twinkle Little Star” -- the more a star twinkles when you observe it, the less stable the atmosphere -- meaning you have poor seeing conditions.
What are the conditions for us to see clearly the stars at night?
Ideal seeing conditions are when there is the least amount of atmospheric disturbances.
The result is sharp, steady views through your telescope.
This can be during hot summer months when the air is heavy and humid or in locations where the topography is flat and there are fewer obstacles for air to interact with..
What causes seeing astronomy?
The seeing effects are caused by atmospheric turbulence through which some of the light arriving from a star is scattered by refractive inhomogeneities.
As the light wave propagates through the atmosphere it experiences fluctuations in amplitude and phase..
What is astronomical conditions?
Astronomical seeing is why objects in the night sky appear to blur and twinkle.
The worse the seeing, the more they blur.
It is changes in the Earth's atmosphere..
What is the best month for stargazing?
Autumn, Winter and Spring offer the best times to stargaze, and many astronomers refer to an 'observing season'.
From the time clocks go back in October (nights become 1-hour longer) to the time they go forward in March (nights become 1-hour shorter)..
What is the scale for seeing conditions?
1 — Very poor images, impossible to see details or to sketch. 2-3 — Almost continuous distortion with occasional brief good moments. 4-6 — More continuous distortions with short intervals of good seeing. 7-8 — Intervals of perfect seeing with fine scale distortions between..
Why do we need astronomy?
By studying the cosmos beyond our own planet, we can understand where we came from, where we are going, and how physics works under conditions which are impossible to recreate on Earth..
- For example poor seeing will almost always occur after a cold front has passed over, replacing the warmer air, with cooler air, which often gives rise to local convection, and turbulent skies.
However, preceding a cold front the air is warmer, and more stable. - Midnight.
This describes when the sun is farthest below the horizon, and corresponds with when the sky is darkest.
Whenever there is no sunrise or sunset, such as near the poles in summer and winter, this describes the time of day when the sky is least bright.
Astronomical Twilight. - seeing conditions are mainly measured in arcseconds, even the scales are sometimes approximated to the arcseconds.
The maximum is divided into a half.
The width in the half of maximum shows the value of seeing as the diagram below show.
It is determined that a bigger value of FWHM means worse conditions for observing. - The cause of degraded or poor seeing is thermal turbulence in the atmosphere.
Seeing has nothing to do with whether the night air is cloudy or clear, warm or cool, or even whether it is windy or calm.
The critical issue is only whether temperature differences in the atmosphere are in motion. - The seeing effects are caused by atmospheric turbulence through which some of the light arriving from a star is scattered by refractive inhomogeneities.
As the light wave propagates through the atmosphere it experiences fluctuations in amplitude and phase.