what is the averagge speed of the Sun in degrees in January and in July?
90071
That would depend on your latitude.  At 90 degrees N in January, the sun is below the horizon so it would be zero degrees per hour whereas at 90 degrees south when the sun is never setting but moving in a circle in the sky, it would be 15 degrees per hour.\n\nThere is no easy formula to figure out the number of degrees per hour at a given latitude.
862790
Yes.  It's highest at noon (not counting Daylight Savings Time) on the first day of summer than any other time in the year.\n\nThis is due to the tilt of the Earth in relationship to the sun.  If you take a globe (or just a beach ball), you can see how it works for yourself.  In the summer, the Earth where you live is tilted towards the sun.  But as the Earth revolves around the sun, the part that's tilted toward the sun in the summer is titled away in the winter.\n\nUse a globe or a ball and walk around a table lamp.  Make sure you hold the globe tilted the same way as you walk around and you'll see what I mean.
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Sunrise and sunset times for Ballyshannon in July \nSunrise 05.00    Sunset 22.00
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The temperature at the centre of the sun is 15 million degrees Celsius, whilst temperatures on the edge of the sun can be as low as 4,000 degrees Celsius. \n\nIt may also interest you to know that a laboratory here on Earth has created a temperature of 510 million degrees Celsius, many times hotter than the hottest part of the sun.
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The Earth orbits the sun at an average speed of 67,000 mph in a counterclockwise direction when viewed from above it's North Pole.
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From Fahrenheit = (value - 32) / 1.80\n\nor use http://www.csun.edu/~jmj2600/hw4.html
450567
The average distance from the Earth to the Sun is 149,597,890 km. Therefore in one year the Earth travels a distance of 2*Pi*(149,597,890)km. This means that the velocity is about: \n\nvelocity=2*Pi*(149,597,890)km/ year\n\nand if we convert that to more meaningful units (knowing there is 365 days in a year, and 24 hours per day) we get: \n\nvelocity=107,300 km/h (or if you prefer 67,062 miles per hour) \n\nSo the Earth moves at about 100,000 km/h around the Sun (which is 1000 times faster than the speeds we go at on a highway!)
1163913
The average distance between the Earth and the Sun is 149,590,787 km or 92,951,640 mi. This distance is called an Astronomical Unit (AU). The orbit of the Earth deviates a bit from a circle, so the distance between the Earth and the Sun isn't always the same. The Earth is closest to the Sun (in the perihelion of the Earth's orbit) around 4 January, when it is winter in the northern hemisphere of the Earth and summer in the southern hemisphere, and is furthest from the Sun (in the aphelion of the Earth's orbit) around 4 July, when it is summer in the north and winter in the south.\n\nThe difference between the distances on 4 January and 4 July is about 3 percent, which corresponds to about 5 million km or 3 million mi.
510653
There are three times a year where Solar time and local time are the same. January, July and then January (ok twice). Determine your position of latitude. Place a short rod in the ground, pointing north at the same angle as your latitude. (pointing to the north star) Make sure the position you pick can be seen from the South by the Sun. Mark the hours off by some smaller rods avery hour of the day. If you do this in January or July you will be closer to real or local time. The shadow of the longer rod, the gnomon, will point to the time rods you have place to mark the shadow. A sundial can also be placed on a vertical wall, with the face to the south, and the "gnomon" point down at the same angle of your latitude.
1169828
The Sun will be closest to the whole planet in January, since that's when Earth reaches perihelion.  However, in January the Northern hemisphere will be tilted away from the Sun.  In July we'll be at aphelion (farthest point from the Sun), but the Northern hemisphere will be tilted towards the Sun and we'll have the longer days (and therefore, summer).
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91.5°East\n\nhttp://en.wikipedia.org/wiki/Measat-1
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i would like to give u this info. : in any country , the summer time begin just after the difference between the dead point of sunrise in winter , then add 60 min. to that time , chk what will be the date of sunset ( +60 min) , then the coming sun. is the date.
1140202
72 degrees Fahrenheit in the summer and 68 degrees Fahrenheit in the winter!
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Use this http://weather.yahoo.com/
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Take a look at this site.  You will need to specify dates and places\n\nhttp://www.weather.gov/climate/
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Finally, the gravitational pull between the Earth and Sun causes the Earth to travel around, or "orbit", the Sun at a velocity of 29.8 km/sec. At the same time, the Earth also turns on its axis causing the daily cycle of day and night. This "rotational velocity" is approximately .47 km/sec. That means that at the same time we're hurdling through space at nearly 67,000 mph, we're also spinning around in circles at over 1000 mph! Whew! Almost makes you dizzy, doesn't it?
1150528
It completely depends on your latitude. You would have to match the earth's rotation rate, one revolution per day. At the equator, that's about 1000 mph, at either pole it's 0 mph, and in between it's between 0 and 1000 mph. (Actually it's about 1000 mph times the cosine of your latitude.) Of course you can range north and south; you don't have to stay at one latitude. But the poles are tricky because of earth's tilt which brings seasonal variations in solar illumination. During spring and summer, at (and near) whichever pole it's spring or summer at, there is no night. \nAs for the mode of transportation, now you know the speed, you can choose.