Has NASA confirmed that a planetary body on a elliptical orbit on the edge of your solar system?
Seeing as how this was written before December 21, 2012, and is probably a reference to the so-called 'Nibiru Cataclysm' involving a massive rogue planet, I can tell you in 2015 that this is not the case. While there are dwarf planets (such as Sedna) orbiting the sun on extremely eccentric paths, there is no gas giant threatening to obliterate Earth. However, as of January 2015, scientists at the Computense University of Madrid claim to have found evidence for two Earth-sized or bigger planets lurking deep in the outer solar system, but the claim at the time of this writing is so new that there is little input from other scientists or corroborative testing by other reputable establishments to give credence to this report.
What is a telescope and how did it help Galileo learn more about the solar system?
Telescopes have allowed us to see further than the naked eye would ever allow. With the invention of the telescope by Hans Lipperhey, mankind has discovered new planets, constellations and threats to our planet such as comets or meteors. Telescopes have also been one of the main reasons that man has begun to explore space, we see things out there worth discovering and taking a closer look at.
The highway system wes derived from plans set forth and implemented by former president Dwight D. Eisenhower. While in office, he structured a project that would change the transportation capabilities for the future. While originally designed and purposed for the national defense system, the highways would provide lanes of which mass transit by military vehicles can travel in case of an emergency and/or military planes have landing and take-of points. The highways also were designed for residents to flee, in case of an emergency, without jamming the rural roadways. It gives residents a direct evacuation route in any direction and can accomodate the mass number of people needing to evacuate.
What object would help us see stars and planets in your solar system more clearly?
a telescope because if you never heard of the Hubble telescope that is like the international telescope.
How is the planet HD 189733b possible?
Planets like HD 189733 b, sometimes called "hot Jupiters" are one of the most common types of planets to be detected, largely because they are the easiest to detect. Such planets likely form at a great distance from their parent stars, but their orbits decay, bringing them extremely close to their stars. Hot Jupiters often slowly lose their atmospheres.
How do planets solar systems and the universe differ?
The inner planets, Mercury, Venus, Earth, and Mars, are mostly rock and iron. The outer planets, Jupiter, Saturn, Uranus, and Neptune, are much larger and are mostly hydrogen, helium, and ice.
The scientist who launched the heliocentric theory on the organization of the solar system is?
I have school on pa cyber i was wondering the same thing
What were the first two space probes to leave your solar system?
Voyager 1 and Voyager 2.
There is a matter of some debate as to whether the two Voyager probes have actually left the solar system, an where the "edge" of the solar system actually is. Both are beyond the orbit of Pluto, but have not passed beyond the vaguely-defined Kuiper Belt, and the two probes are just approaching the heliopause, the boundary layer between the solar wind and the broader currents of interstellar space.
But it seems likely that however that boundary is defined, the two Voyager probes either were or will be the first man-made objects to pass it.
What is a good name for a alien from Uranus?
-- Ralph
-- Bertrand
-- Gulliver
But rather than give him a name we've chosen, before we ever knew anything
about him, wouldn't it be a much friendlier gesture to try to find out what name
he calls himself ?
Why are the planets spread out like they are?
because where they are today is where they formed. by where they are i mean how far away they are from the sun. but the universe is always changing.
What naked eye planets that NEVER appears next to a full moon Venus Mars Jupiter Saturn?
Inferior planets (Mercury and Venus) can never be opposite to the Sun, since they are nearer to the Sun than we are. Therefore, it follows that they can't be seen next to a full moon, which is opposite to the Sun in the sky.
Well, you don't want to send a probe to one location in space where a planet doesn't obit, it would be pointless. So knowing the orbits of the planets help you send whatever you're trying to send to the right location, and not just a random spot in space.
What makes the planets have different temperatures?
Their distance from the Sun and the composition of their atmospheres.
The terrestrial planets (Mercury, Venus, Earth, and Mars) receive heat from the Sun and radiate some back into space. Mercury has no appreciable atmosphere and experiences the highest range of temperatures simultaneously. Venus has a dense atmosphere that retains heat (too hot), and Mars has a thin atmosphere that loses most of its heat (too cold). The Earth is in the fortunate middle range for solar radiation and atmospheric density.
The gas giants (Jupiter, Saturn, Uranus and Neptune) receive comparatively little solar heat, which makes their outer atmospheres very cold. But their (deep and unseen) surfaces are heated to thousands of degrees by the massive pressure of their atmospheres.
Earth and Solar Radiation
The "Solar constant" is the average amount of sunlight that crosses a unit area every second. A recent estimate from satellite observations is 1,366 watts per square meter.
From the fact that Earth receives sunlight on its cross-sectional area (pi R^2), but has an actual area four times larger (4 pi R^2), we can see that the average sunlight falling on a square meter of the Earth is 341.5 watts per square meter. But the Earth reflects some of this right back out to space -- 30.6% according to NASA. So the sunlight entering the Earth's climate system averages 237 watts per square meter.
Energy is conserved. Earth must radiate back out as much as it receives. From the Stefan-Boltzmann relation, which says the flux density coming out of a radiating object is proportionate to the fourth power of temperature (times the "Stefan-Boltzmann constant" of 5.6704 x 10^-8 watts per square meter per kelvin to the fourth), that 237 watts per square meter corresponds to a temperature of 254 K. This is Earth's "radiative equilibrium temperature."
But water freezes at 273 K, so if equilibrium temperature were the whole story, Earth would be frozen over! But greenhouse gases in its atmosphere -- primarily water vapor and carbon dioxide -- bring the surface temperature up to 288 K, an increase of 34 K. Calculating how the greenhouse effect works is much more complicated than finding the radiative equilibrium temperature, but there are ways to do it.
For those who like formulas, here are a few to remember:
Flux input to the climate system: Fin = (S / 4) (1 - A) where S is the solar constant and A the planet's "bolometric Bond albedo."
Conservation of energy: Fin = Fout
Equilibrium temperature (also called effective temperature or emission temperature): Te = (Fout / sigma) ^ 0.25 where sigma is the Stefan-Boltzmann constant.
Greenhouse temperature increment: Tg = Ts - Te where Ts is the surface temperature.
Mars and Venus are good examples for comparison. For Venus, S = 2611 watts per square meter, A = 0.750 according to NASA, so Fin = Fout = 163 watts per square meter and Te = 232 K. For Mars, S = 589 W/m^2, A = 0.250, F = 110 W/m^2 and Te = 210 K. Note what a big difference the greenhouse effect can make: For Mars, Ts = 214 K, so Tg is 4 K, caused by Mars's thin carbon dioxide atmosphere. For Venus, Ts = 735 K (!), leading to Tg = 503 K, a huge difference due its very thick carbon dioxide atmosphere and sulfuric acid clouds.
The equilibrium temperature model breaks down for the giant planets, which have internal heat sources.
Why is Uranus and Neptune not included in the heliocentric and geocentric model of the solar system?
The planets Uranus and Neptune were discovered only in modern times after the heliocentric model had been generally accepted.
The Sun has more gravity than the other planets in your solar system because the Sun is?
... more massive (it has more mass).
... more massive (it has more mass).
... more massive (it has more mass).
... more massive (it has more mass).
What is oure system of dating centered on?
a group of people that invaded India and developed the caste system
A solar system object of rocky composition and comparable in size to a small city is most likely?
ASTROID!
Our unique solar system how it got here?
There is probably nothing unique about our solar system. Scientists once thought that planets might be rare, but we're finding that planets appear to be as common as dirt; we know of over 400 "exoplanets" circling other stars.
So far, our technology isn't good enough to locate a planet as small as Earth, but with big planets as common as they are, there's no reason to think that "ordinary" worlds will be any more rare.
Why does the geocentric system use epicycles when the heliocentric does not?
The geocentric system uses epicycles in order to create a model in which the earth is in the center of the solar system and the planets and sun look the way they actually look from the earth with the naked eye. The idea of epicycles was added by Ptolemy because without them his model was not consistent with what the ancients recorded about the position of the planets, the sun and the moon. It was important that the model be consistent with observation since the model was used for navigation and land travel. Once the telescope came into being it was evident that the geocentric model (which included the epicycles) was not consistent with was now observable in the sky, such as the way that Venus looked at different times of years (the phases of Venus). Therefore the geocentric model was abandoned for the heliocentric model. The heliocentric model's predicted movements that were closer to what was observable with the new technology. The heliocentric model does not "need" epicycles, in fact they would lead to false predictions inconsistent with what was observable.
How many planets can a solar system have according to the nebular theory?
There is no maximum number, and "nebular theory" has been knocked for a loop by the recent discoveries of 400+ "extra-solar planets" - planets orbiting other stars.
Classical theories predicted that planetary systems would be rare; however, it seems that every nearby star we've looked at recently has been discovered to have planets - LOTS of planets.
According to modern understanding, the planets, and the Sun, move around the Solar System's center of mass. Since the Sun is much more massive than the planets, this center of mass is very close to the Sun.
If the Sun is much larger than any of the planets, it seems likely that it also has a greater mass - assuming that their respective densities are somewhat similar. And indeed, this is the case here.
What holds the galaxies and solar systems together?
Galaxies are held together by gravity. So are Solar Systems. In the case of galaxies, and galaxy clusters, it isn't entirely clear what type of masses provide this gravity - the amount of known matter is simply too small, by a factor of 5-10. For more information, do some reading on "dark matter".
Why did the 7 dwarfs mine for diamonds?
The oldest versions of that tale don't say what they mined for, only that they were miners.
Disney probably had them mine for "diamonds" because hey, why not, the notion of there being gems in a mine is simpler to draw than them extracting ores (rock of a slightly different color from the surrounding rock) and then smelting it into metals. They could have mined gold, I suppose; gold is found uncombined.