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Our Solar System -- What We See

Introduction
Ionospheres/Plasma spheres
The Sun
The Inner Planets
The Outer Planets
The Asteroid Belt
The Kuiper Belt
Craters
Things that Fly Through the Sky
Comet 67P

Explanations and Interpretations

Introduction:

Our solar system is a very small part of our whole Milky Way Galaxy. We are in one of its spiral arms.

solarsystem in galaxy

Our solar system is made up of five parts: the sun, the inner four planets, the outer four planets, the asteroid belt and the Kuiper belt.

solarsystem

 

The illustration below shows the relative sizes a little more clearly.

comparisons

If you look very hard next to the earth, you will see a tiny dot. That is our moon. Then why can the moon block the sun during an eclipse? Pick up a leaf.  Hold it up and see how much of a distant tree you can block out with the leaf.  Does that mean the leaf is bigger than the tree? We are far enough away from the sun for the moon to look like it is the same size to us.  That is why the moon can cover the sun during a solar eclipse

eclipse

Understanding that distance really makes things look smaller, let’s look at some of the sizes in numbers:

Let’s make the earth 1 inch wide.
Our moon would be ¼ of an inch wide.
Jupiter would be 11 inches wide.
The sun would be 125 inches wide (almost 10 ½ feet).
Our galaxy, the Milky Way, would be  about 6 x 1011 inches (600,000,000,000 inches) or   9.3 MILLION miles across

Here's something to try to help you understand these distances: How far would you have to back up from the sun (if it were 10.5 feet across)  so that the moon (1/4 inch across) could cover it?  Try it.  It will take more than your yard.  It will take more than a store's parking lot.  Mark off a colored tape along two posts that are 10.5 feet apart, and walk down a long, straight road with your quarter inch moon. Keep trying to block out the tape with the moon.  That will give you an idea of how far our moon is from our sun.

Ionospheres/Plasmaspheres

Every planet in our solar system is surrounded by an ionosphere, also known as a plasma sphere or an magnetosphere. This is a very large surround of ionized gases which deflects the solar wind away from the planets themselves.

plasmasphere2

Ions are atoms which have been stripped of one or more electrons. This produces a positive charge in the atom itself and the freed electrons produce negative charges. This is also known as 'plasma' or the fourth state of matter. The Plasma Model explains this more fully. The bow shock is where the solar wind hits the front of the plasma sphere and is deflected to the sides. The solar wind is a positively charged electric current, primarily protons. The planet's own magnetic field (giving it a north and south pole) results in weak spots where some solar wind can enter. These are called cusps. When the solar wind is strong enough due to some kind of 'burst' from the sun (see below), then the planet's plasma sphere at the poles will react to the added electric current and go into glow mode and show up as auroras.

Every electric current is surrounded by a magnetic field circling it. This is explained in the Plasma Model, linked in the previous paragraph. An electric current is either negative, involving a stream of moving electrons or positive, involving a stream of moving ions or protons. If there were no solar wind, the magnetosheath would be in a large globe around the planet. However the force from the solar wind causes it to stream out behind the planet like a giant wind sock. The magnetopause is where the interaction with the solar wind actually stops, and then we proceed further in to the lobes and magnetotail, which are the streaming parts of the magnetosphere (plasmasphere).

The trapping region is where ions are trapped. The planet's magnetic field itself produces the trapping region where electrons and ions spiral around the planet itself, again showing dips or weaknesses at the two poles. The narrow neutral sheet is a merging of the magnetic fields of the north and south poles where there is no positive or negative charge.

The plasma sphere/ionosphere tails stream out for exceedingly long distances and the next planet out is quite capable of passing through it. Saturn can pass through Jupiter's; we can pass through Venus'; Mars can pass through ours, etc. It is important to note that there are three names for these things: ionospheres, magnetospheres, and plasma spheres. All are correct.

magnetospheres

Not only does each planet have its own plasma sphere, our entire solar system is surrounded by a very large one, which is the sun's plasma sphere. It is called a heliosphere.

heliosphere

 

The solar apex is the direction in which the solar system is moving in space. The interstellar wind is similar to the solar wind from the sun. It is the combination of the output of the various stars in our part of the Milky Way Galaxy and the interstellar magnetic field. The bow shock is where the interstellar wind hits and is forced around the solar system. The heliopause is where interaction with the interstellar wind stops. The heliosphere is explained well by Wikipedia:

The heliosphere is the region of space dominated by the Sun. The edge of the heliosphere is a magnetic bubble-like medium and is located far beyond the orbit of Pluto. Plasma "blown" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical.

May, 2015 -- massive solar flare

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