As we know the stars as viewed from the earth are not seen as in their actual position due to atmospheric refraction.But in this method we calculate the distance to...
1 Answers 1 viewsFor your long-term-memory: If $alpha$ radian is the parsec angle, the formula for distance = 1/$alpha$ AU. Here, $alpha$=(0.379/3600)($pi$/180) radian.=1.8374 E-06 radian. So, d=1/1.8374 AU=544000 AU. Unit conversions: In lu...
1 Answers 1 viewsA telescope allows us to see more stars in a limited region. By having more stars to look at, we have a better chance of seeing them shift in the...
1 Answers 1 viewsThe angle has to be in second ( '' ) unit. For 1'' parallax angle, the distance is 1 parsec. For other values in seconds, the distance = 1/(angle in...
1 Answers 1 viewsI assume that the unit for angle is 1 degree. By definition of parsec, for parallax angle 1sec, the distance is 1 parsec. So, for $0.002790^o= 0.002790 X 3600...
1 Answers 1 viewsdistance= 1/ parallax in arc secs. 1/.0012293 773.34 parsecs.
1 Answers 1 viewsThe distance of a star with parallax 1 arc sec is 1 parsec. The distance of a star with parallax k arc sec is k parsec. 1 parsec = 206265...
1 Answers 1 viewsThe relationship between a star's distance and its parallax angle is given by $d = 1/p$, where the distance $d$ is measured in parsecs (equal to $3.26$ light years) and...
1 Answers 1 viewsSymmetry can sometimes be used to interpret an NMR spectrum, , and also The above treatment will tell you HOW many signals you should see in the spectrum; it...
1 Answers 1 viewsAdsorption spectroscopy measures the amount of a wavelength adsorbed by a substance. Emission spectroscopy measures the amount of a wavelength emitted by a substance after excitation. In both versions,...
1 Answers 1 views