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Constellations - Javalab
Constellations - Javalab
Constellations If you look at the sky where there is no light on a clear night, there are so many stars that can not count. Thousands of years ago, the ancients linked stars to create constellations named after animals, objects, and mythical figures. Each star in the constellation is only…
·javalab.org·
Constellations - Javalab
Distance of 1 pc(parsec) - Javalab
Distance of 1 pc(parsec) - Javalab
Parallax When an object is close to me, you can use a ruler to measure the distance. But, it isn't easy to measure when the object is away from me. In this case, how can you measure the distance? Humans have two eyes. The world with the left eye and…
·javalab.org·
Distance of 1 pc(parsec) - Javalab
Scale of Solar System - Javalab
Scale of Solar System - Javalab
Press the button of the planet you want to go. Orbital radii of the planets has applied the average.
·javalab.org·
Scale of Solar System - Javalab
Diurnal Motion of Sun - Javalab
Diurnal Motion of Sun - Javalab
* If you are asked to access your location, please allow it. * Your personal data is not stored on the server. * For iOS devices, please allow location access as follows. Diurnal Motion Fix the camera towards Polaris at night, shoot for a few hours, and you'll see the…
·javalab.org·
Diurnal Motion of Sun - Javalab
Tidal Force - Javalab
Tidal Force - Javalab
Tidal force Earth is not an object like a point (· ), but a rigid body (●) with a certain volume, so the gravity applied to each part is slightly different. This difference in gravity applies to all celestial bodies of volume. In the case of the Earth, only seawater…
·javalab.org·
Tidal Force - Javalab
Tides - Javalab
Tides - Javalab
Tide is a phenomenon that the ocean surface's periodic rise and fall due to the moon and sun's gravitational pulls. Spring Tide is the highest high tide that occurs during the tide. It occurs when the Sun, Earth & Moon are in a straight line. Neap Tide is a tide…
·javalab.org·
Tides - Javalab
Foucault Pendulum (WebGL) - Javalab
Foucault Pendulum (WebGL) - Javalab
Foucault's pendulum is a device invented by French scientist Leon Foucault to prove the Earth's rotation in 1851. The fact that the Earth rotates has been known for a long time, but it is the first example that proves it by experiments. Foucault's pendulum is a freely swinging pendulum whose…
·javalab.org·
Foucault Pendulum (WebGL) - Javalab
Latitude of Polaris - Javalab
Latitude of Polaris - Javalab
Latitude of Polaris Polaris is far from Earth. Thus, light from the North Star reaches parallel to the Earth. And since the earth is round, the North Star's latitude varies depending on where it is observed. Incidentally, the North Star is located in an extension of the Earth's axis of…
·javalab.org·
Latitude of Polaris - Javalab
Real Size & Orbit of Earth and Moon - Javalab
Real Size & Orbit of Earth and Moon - Javalab
The photographs of the Earth and the moon close together that you can see on posters, etc., are designed to be easy to see. The moon's apparent diameter is only about 0.5˚. This tells us that the Earth and the Moon are pretty far apart than you thought. With the…
·javalab.org·
Real Size & Orbit of Earth and Moon - Javalab
Earth's Revolution and Seasons (WebGL) - Javalab
Earth's Revolution and Seasons (WebGL) - Javalab
Earth Rotation and Seasonal Changes The Earth's rotation axis is tilted at an angle of about 23.5 ° to the orbital axis. Because of this inclination, seasonal changes occur like spring, summer, autumn, and winter. The sun illuminates the northern hemisphere more in June-August. So, the northern hemisphere becomes summer,…
·javalab.org·
Earth's Revolution and Seasons (WebGL) - Javalab
Day and Night, Seasons, White Night, Polar Night - Javalab
Day and Night, Seasons, White Night, Polar Night - Javalab
* If you are asked to access your location, please allow it. * Your personal data is not stored on the server. * For iOS devices, please allow location access as follows. Day and night The earth is spherical, so only half of the earth's surface receives sunlight. Daytime is…
·javalab.org·
Day and Night, Seasons, White Night, Polar Night - Javalab
Zodiac - Javalab
Zodiac - Javalab
Zodiac The Ecliptic is the way the sun passes in the sky. zodiac means 12 constellations on the ecliptic. It is said that the zodiac was made in Babylonia around the 7th century BC. Constellation 1 - Aries : March 21 - April 19 Constellation 2 - Taurus : April…
·javalab.org·
Zodiac - Javalab
Kepler's law - Javalab
Kepler's law - Javalab
Kepler and Tycho Brahe There is an astronomer before talking about Kepler (Johannes Kepler 1571 ~ 1630). That's Tycho Brahe. Tycho Brahe (1546-1601) is a famous Danish astronomer. With the development of astronomical equipment, he left a vast amount of information about the stars' location, and he made a great…
·javalab.org·
Kepler's law - Javalab
Equatorial Coordinate System - Javalab
Equatorial Coordinate System - Javalab
Celestial coordinate system A celestial sphere is an abstract sphere centered on an observer. All objects in the sky can be conceived as projected upon the celestial sphere's inner surface. Equatorial system The equatorial coordinate system is the most basic coordinate system around the Earth. Most celestial bodies use this…
·javalab.org·
Equatorial Coordinate System - Javalab
Geocentrism vs. Heliocentrism - Javalab
Geocentrism vs. Heliocentrism - Javalab
Geocentrism, The Geocentric theory The Geocentric theory is a cosmic perspective in which the Earth is at the center, and all the stars revolve around the Earth. From the 13th to the 17th century, it was a widely recognized worldview in Christian societies, including the Roman Catholic Church. Heliocentrism, The…
·javalab.org·
Geocentrism vs. Heliocentrism - Javalab
Elevator Ride
Elevator Ride
This collection of interactive simulations allow learners of Physics to explore core physics concepts by altering variables and observing the results. This section contains nearly 100 simulations and the numbers continue to grow.
·physicsclassroom.com·
Elevator Ride