Local Sidereal Time Solution

STEP 0: Pre-Calculation Summary
Formula Used
Local Sidereal Time = Greenwich Sidereal Time+East Longitude
LST = GST+Elong
This formula uses 3 Variables
Variables Used
Local Sidereal Time - (Measured in Radian) - Local Sidereal Time is a concept primarily used in astronomy and celestial navigation. It refers to the time measured with respect to the local meridian and the position of the stars.
Greenwich Sidereal Time - (Measured in Radian) - Greenwich Sidereal Time (GST) is a concept used in astronomy and celestial navigation to measure the rotation of the Earth relative to the stars.
East Longitude - (Measured in Radian) - East Longitude refers to a specific geographical location on the Earth's surface in relation to the prime meridian, which is designated as 0 degrees longitude.
STEP 1: Convert Input(s) to Base Unit
Greenwich Sidereal Time: 96 Degree --> 1.67551608191424 Radian (Check conversion ​here)
East Longitude: 15 Degree --> 0.2617993877991 Radian (Check conversion ​here)
STEP 2: Evaluate Formula
Substituting Input Values in Formula
LST = GST+Elong --> 1.67551608191424+0.2617993877991
Evaluating ... ...
LST = 1.93731546971334
STEP 3: Convert Result to Output's Unit
1.93731546971334 Radian -->111 Degree (Check conversion ​here)
FINAL ANSWER
111 Degree <-- Local Sidereal Time
(Calculation completed in 00.006 seconds)

Credits

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Created by Shobhit Dimri
Bipin Tripathi Kumaon Institute of Technology (BTKIT), Dwarahat
Shobhit Dimri has created this Calculator and 900+ more calculators!
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Verified by Urvi Rathod
Vishwakarma Government Engineering College (VGEC), Ahmedabad
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Local Sidereal Time Formula

​LaTeX ​Go
Local Sidereal Time = Greenwich Sidereal Time+East Longitude
LST = GST+Elong

What is the use of Sidereal time?

Sidereal time is used by astronomers to determine where a certain heavenly body will appear in our sky at any given time. Star positions are described in terms of declination and right ascension, and right ascension is measured in units of sidereal time.

How to Calculate Local Sidereal Time?

Local Sidereal Time calculator uses Local Sidereal Time = Greenwich Sidereal Time+East Longitude to calculate the Local Sidereal Time, Local Sidereal Time (LST) is the measure of the hour angle of the vernal equinox at a specific location, indicating the position of the Earth relative to the fixed stars, important in astronomy and celestial navigation. Local Sidereal Time is denoted by LST symbol.

How to calculate Local Sidereal Time using this online calculator? To use this online calculator for Local Sidereal Time, enter Greenwich Sidereal Time (GST) & East Longitude (Elong) and hit the calculate button. Here is how the Local Sidereal Time calculation can be explained with given input values -> 6359.832 = 1.67551608191424+0.2617993877991.

FAQ

What is Local Sidereal Time?
Local Sidereal Time (LST) is the measure of the hour angle of the vernal equinox at a specific location, indicating the position of the Earth relative to the fixed stars, important in astronomy and celestial navigation and is represented as LST = GST+Elong or Local Sidereal Time = Greenwich Sidereal Time+East Longitude. Greenwich Sidereal Time (GST) is a concept used in astronomy and celestial navigation to measure the rotation of the Earth relative to the stars & East Longitude refers to a specific geographical location on the Earth's surface in relation to the prime meridian, which is designated as 0 degrees longitude.
How to calculate Local Sidereal Time?
Local Sidereal Time (LST) is the measure of the hour angle of the vernal equinox at a specific location, indicating the position of the Earth relative to the fixed stars, important in astronomy and celestial navigation is calculated using Local Sidereal Time = Greenwich Sidereal Time+East Longitude. To calculate Local Sidereal Time, you need Greenwich Sidereal Time (GST) & East Longitude (Elong). With our tool, you need to enter the respective value for Greenwich Sidereal Time & East Longitude and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
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