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Meridiano di Greenwich

Il  meridiano di Greenwich  (o  meridiano fondamentale  o  meridiano primo  o  meridiano zero ) è il circolo massimo meridiano avente per convenzione longitudine zero. This is the line of longitude passing through the Greenwich Observatory in England.

It was agreed in October 1884 in Washington with the President of the United States of America, 41 delegates from 25 countries gathered for the International Meridian Conference.

Tool to find the coordinates (latitude and longitude) in Google Maps

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Latitudine e Longitudine

The longitude (Latin longitudinal , longitudĭnis , "long" derivative longus, "long") is the geographical coordinates showing the angular distance east or west in direction from the prime meridian. This angle is measured in sexagesimal degrees in a plane perpendicular to the ground and can take values \u200b\u200bin da 0 a 180° E e da 0 a 180° W.

La  latitudine  (o  latitudine geografica ) è la coordinata geografica pari all'altezza del polo celeste sull'orizzonte. La latitudine è pari all'angolo che la verticale di un punto sulla superficie della Terra (o di un pianeta) forma con il piano equatoriale. Tale angolo viene misurato in gradi sessagesimali e può assumere valori nell'intervallo da 0 a 90° N e da 0 a 90° S.

Click here to read the entire article L ongitudine on wikipedia.

Click here to read the entire article L atitudine on wikipedia.

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LEZIONI DI FRANCESE

IMPORTANT NOTICE: THERE
'OPPORTUNITY' TO WORK ON THIS BLOG ALSO WITH THE PROFESSOR OF FRENCH.
WHAT THEY SAY AND DO YOU THINK?

TO START VISIT:
WWW.TVCINQUE.FR

PROF. ANGELO COPPOLA

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Il metodo scientifico

The scientific method is the typical way in which science proceeds to reach a knowledge of reality objective , reliable, verifiable and shared . It consists, first, in the collection of empirical evidence and measurable through observation and experiment, on the other, in the formulation of hypotheses and theories to be examined again to experiment.

click here to read the entire article scientific method on Wikipedia

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1. THE LAW OF UNIVERSAL GRAVITATION


Legend has it that the idea of \u200b\u200bthe law of gravity comes to Newton watching an apple fall from a tree (other versions give the apple fall directly on his head), Newton would asked what would happen if the apple had fallen from a height equal to the distanza tra la luna e la terra. Si accorse dunque che la mela e la luna, questi due oggetti così diversi tra loro, potevano ugualmente essere soggetti alla stessa legge fisica. In realtà la formulazione della legge di gravità è l'ultimo atto di un lungo percorso scientifico che aveva portato numerosi fisici prima di Newton ad analizzare solo parzialmente le leggi della dinamica dei corpi a seguito delle scoperte di Galileo .
Newton scoprì che le masse dei corpi celesti si attraggono proporzionalmente al prodotto delle masse e in ragione inversa del quadrato delle distanze, tale attrazione prese il nome di gravità. Questa legge, semplice in sé, comportava una rivoluzione epocale nella meccanica dei corpi, la gravità was universally valid in all places of the universe and suggested a reciprocal relationship and mutual influence of all bodies in the cosmos. Gravity is the force that a body on the ground is still held to the ground. More mass, the greater will be its gravitational pull, and nothing that has a mass less may be released by the gravitational pull of the greatest mass, except with great effort (think of the enormous amount of energy needed to detach from ground rockets and let them escape the Earth's gravity). In light of the new theory, the elliptical motion of the stars of Kepler was questioned, since the ellipses describing the Earth around the Sun could not be sustained as perfect as the study of Kepler, but he should submit to the influence of disturbances resulting from the mass of other planets.
The universe described by Newton possessed the quality of being uniform in an absolute sense. This means that each region of space-time universe is not only subject to the same physical laws, but also had a level playing time and geometric space and time which will then be put into question the theory of relativity. The classical physics of Newton still involved the necessary presence of the ether, the presence of a light material that was still volatile and almost occupy all spaces of the cosmos to make possible the transmission of physical and mechanical causes and effects of all phenomena (the story of the refutation of the ether see Einstein's relativity ).
2. Mass and Weight
The definition of the law of gravity implies the distinction between mass and weight of a body: the mass of a body is the amount of matter present in the body, according to the quantity which forms the force of gravity and the weight Instead of a body is the result of the gravitational force applied on the body. The farther away from Earth, which is the largest agglomeration of matter "in the immediate vicinity" of man, the strength of gravity exerted by the planet on the bodies decreases, which is why astronauts have envy gift of weight loss and soaring into space. The mass is then quell'agglomerato of matter that makes it possible for gravity to exert a certain force of attraction, and the weight is simply the effect of this force (on the moon, the bodies are lighter because it is less mass to attract If the bodies in a more bland).
Again, as already seen for Galileo, the new scientific method not only allows you to reach conclusions that go beyond common sense, but also allows to predict the behavior of extraordinary bodies in unexplored regions of space (the astronauts necessarily suffer the effects of that law of gravity was discovered that the first three centuries of their experiences in weightlessness).



EMANUELE GRAMAGLIA.

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Isaac Newton e la sua legge della gravità

" Any object Universe attracts every other object with a force directed along the line joining the centers of gravity of the two objects , intensity directly proportional to the product of their masses and inversely proportional to the square of their distance " .

Isaac Newton

click here to read the full article gravity on Wikipedia

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la forza di gravità e le leggi di Keplero

The law of gravity

Gravity is one of the four fundamental interactions governing the entire universe . In classical mechanics gravity turns out to be a conservative force that occurs between bodies with mass , and therefore has a ' gravitational potential energy , in theory Ria of general relativity gravity is instead linked to the geometry (non-Euclidean) space-time of and deviates from the straight course, including massless particles, such as the foton .

Kepler's Laws

The three laws of planetary motion are the main contribution of Johannes Kepler, Kepler said, to ' astronomy and mechanics . Kepler derived in part by studying the observations of Tycho Brahe . Isaac Newton was later verified the validity of these laws in light of theory of universal gravitation .

FIRST LAW
L ' orbit described by a planet is an ellipse , whose Sun occupies one of two fires .

SECOND LAW

The radius vector joining the center of the Sun with the center of the planet describes areas in equal times equal.

THIRD LAW

The squares of revolution periods of planets are directly proportional to the cubic and semi-major axes of their orbits.

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KEPLERO E NEWTON

PROF. RIGOLI G.

HELLO, BOYS!
we are studying Kepler's laws?
EVEN IF YOU DID NOT GET STARTED NOW.
and insert images that explains how to MOVE The planet around the sun.
Next: Gravity '
AND THE LAW OF NEWTON.

The orbits of the planets are ellitticheGiovanni Kepler (1571-1630), astronomo tedesco, derivò le tre leggi del moto dei pianeti che successivamente influenzarono le idee di Newton quando ricavò le leggi della gravitazione universale. Nel 1597 Keplero pubblicò il Mysterium cosmographicum che lo fece conoscere al grande astronomo Tycho Brahe e a Galileo Galilei.Durante il suo soggiorno a Praga, tra il 1600 e il 1611, egli calcolò l'orbita di Marte e ricavò le prime due leggi del moto dei pianeti.Nel 1619, Keplero pubblicò la terza legge che assieme alle prime due furono descritte nella sua opera maggiore, l'Epitome astronomiae copernicanae, edita in sette libri dal 1618 al 1621. L'opera di Keplero ebbe una grande influenza nell'astronomia del Seicento.