Yesterday should be the hottest day.Masa tengah hari memang terasa panas sangat.Kepala pon dah pening2.Masa aku tengah isi minyak tengah hari semalam, ada sorang chinese guy ni tegur aku.
"Haiya...manyak panas hari ni. Saya sudah minum banyak air pon tak tahan juga". Aku senyum jer tengok dia. memang padan la dia terasa panas. Sebab dia naik motosikal jer.Kalau naik kereta mungkin kurang rasa panasnya sebab ber aircond.
Ku ingat panas hingga ke malam, rupanya petang tu hujan turun lebat.so hari yg panas jadi hari yg sejuk. kat area rumah aku ni memang panas setiap masa.Kalau tido pon bukak kipas sampai level 5.Tu pun tak cukup lagi nak sejukkan bilik tu.Bangun pagi wajib badan berpeluh2.Tapi semalam memang sejuk.Tak payah bukak kipas pon takper.Ahaha, hari yg patut panas sangat jadi hari yg sejuk dalam sejarah aku duk umah kat puchong ni.
Some info about this equinox:
In astronomy, an equinox is defined as the moment when the sun reaches one of two intersections between the ecliptic and the celestial equator.
The word "equinox" comes from the Latin for "equal night". The equinoxes in March and September are the two occasions each year when the day and the night are of equal duration. For measuring the length of a day, sunrise is the moment when the sun is half-above the horizon and sunset is the moment when the sun is half-under the horizon. Using this definition, the length of the day (and the night) is precisely 12 hours at an equinox.
In the northern hemisphere, the March equinox is known as the vernal (spring) equinox and the September equinox is the autumnal (autumn) equinox. In the southern hemisphere, these names may be transposed.
The vernal equinox typically falls on either 20 or March 21 and the autumnal equinox on 22 or September 23 � the dates vary because some years are leap years, shifting the calendar by a day or so relative to the seasons. Because the Earth's orbit is elliptical, the dates on which the equinoxes fall do not divide the year into equal halves.
The equinoxes can also be interpreted as virtual points in the sky. Although, during full daylight, stars other than the sun are overwhelmed by sunlight, making it hard to see where the sun is compared to other celestial bodies, the sun does have a position (as seen from the earth) relative to the other stars. As the Earth moves around the sun, the apparent position of the sun relative to the other stars moves in a full circle over the period of a year. This circle is called the ecliptic, and is also the plane of the Earth's orbit projected against the whole sky. The other bright planets like Venus, Mars and Saturn, also appear to move along the ecliptic, because their orbits are in a similar plane to Earth's.
Another virtual circle in the sky is the celestial equator, or the projection of the plane of the Earth's equator against the whole sky. Because the Earth's axis of rotation is tilted relative to the plane of Earth's orbit around the sun, the celestial equator is inclined to the ecliptic. Twice a year, the sun, making its progress around the ecliptic, crosses the plane of the Earth's equator. These two points are the equinoxes. The time at which the sun passes through each equinox point can be calculated precisely�so the equinox is actually a particular moment, rather than a whole day.
8:03 a.m. - March 22, 2005
Recent entries:
January 05, 2018 : -
August 31, 2006 : The End
August 31, 2006 : Keranamu Malaysia
August 28, 2006 : Weekend!
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