Not sure what you mean by "time difference". If humans ever go near that planet, they would probably use Earth time, and that would probably be UTC.
The planet Venus is _NEVER_ seen in the full phase, because it never gets anywhere near the Earth. Venus is in a closer orbit to the Sun than the Earth is, so when Venus is closest to the Earth, it's pretty close to being between the Earth and the Sun. In fact, Venus passes directly between the Earth and the Sun twice per century, most recently in 2004. We call this a "transit of Venus".So we only see Venus in its crescent phases.Think about it . . . In order to see the complete illuminated side of Venus,we'd have to be looking at it through the sun.
It is closer to the Sun.
You are confused. "Light-year" is a measurement of DISTANCE, the distance that light travels in one year; it is not a time period. Venus is, depending on where Venus and Earth are in our respective orbits, between 2 and 14 light-minutes away; light would take somewhere between 2 and 14 minutes to span the distance. You can convert easily minutes into years; there are 60 minutes in an hour, 24 hours in a day, and 365.26 days in a year.
There is a two hour time difference between Colorado (Mountain Time) and Pennsylvania (Eastern Time). Example: 8 AM in Colorado = 10 AM in Pennsylvania.
there is a time difference between all the parts of the world as the sun revolves fromwest and that is why the time is ahead in the east and behind in the west . if a meridian passes through a place , all the places that come in the path of that meridian have the same time .the time difference is not much in between the meridian s . these regions are known as TIME ZONES .a time selected for a particular place at noon is known as that pace's LOCAL MEAN TIME
Venus and the Earth both have very nearly circular orbits round the Sun, but Venus's orbit has a smaller diameter. Since the two orbits are nearly in the same plane, and Venus goes round more quickly than the Earth, it follows that Venus must pass between the Earth and the Sun every time it overtakes the Earth. Venus does approximately 365 revolutions in the time taken by the Earth to do 225. Because the two planets' orbits are slightly inclined, the three object are lined up exactly quite infrequently, but sometimes Venus passes between Earth and Sun and can be seen as a black dot crossing the face of the Sun in what is called a transit of Venus.
The longest time zone difference between two locations on Earth is 26 hours.
The maximum time zone difference between two locations on Earth is 26 hours.
The concept of a 24 hour day cannot be extended to Venus or Mercury as it is to Earth and Mars. On Earth, there is only a tiny difference between rotational time and solar time. On Venus, the difference between the sidereal day (243 Earth days) and the solar day (117 Earth days) makes clock times meaningless.A rotational day on Venus takes about 5832 Earth hours. A sunrise-to-sunrise day takes about 2802 Earth hours. Using either to design a clock would not be practical. Even the defining characteristic of day and night are not important because radar is used to observe the surface beneath the clouds. There is also virtually no difference between day and night temperatures on the surface.One concept that is used for time on Venus is the longitudinal noon, which establishes 360 divisions of rotational time to the 1.92 solar days that exist during the Venusian year (225 Earth days). Of course, the Sun would never actually be visible on the surface.
Venus has a shorter travel time in light years from Earth compared to Jupiter. The distance between Earth and Venus can range from about 0.28 to 0.69 light minutes, while the distance to Jupiter ranges from about 32 to 53 light minutes.
The greatest time difference between two points on Earth is 26 hours. This occurs between the Baker and Howland Islands in the Pacific Ocean.
15.5 hrs
no it does not
The planet Venus is _NEVER_ seen in the full phase, because it never gets anywhere near the Earth. Venus is in a closer orbit to the Sun than the Earth is, so when Venus is closest to the Earth, it's pretty close to being between the Earth and the Sun. In fact, Venus passes directly between the Earth and the Sun twice per century, most recently in 2004. We call this a "transit of Venus".So we only see Venus in its crescent phases.Think about it . . . In order to see the complete illuminated side of Venus,we'd have to be looking at it through the sun.
The sidereal day is about 243 Earth days. That is the time for the planet to rotate once . The solar day is 117 Earth days,roughly. That is a big difference. On Earth the difference between these two days is only about 4 minutes. The reason for the big difference on Venus is that Venus rotates very slowly. The solar day depends on the rotation of a planet AND its orbital motion. The slow rotation makes the effect of the orbital motion much greater on the length of the solar day. Incidentally Venus rotates in the opposite direction to Earth. That's why the solar day is shorter than the sidereal day. On Earth it's the other way round.
The maximum time difference between two locations on Earth is 24 hours, which occurs when they are on opposite sides of the International Date Line.
The largest time zone difference between two locations on Earth is 26 hours. This occurs between Baker Island and the Line Islands in the Pacific Ocean.