Universe

Planetary Detection Rapid

The planetary detection rapid is a technique that we can use to help detect new planets and moons when travelling through interstellar space.


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Planetary-Detection

Introduction

The planetary detection rapid is a technique that we can use to help detect new planets and moons when travelling through interstellar space. The way that the detection system works is by sending out an energy rapid and when it hits a planet or moon the way that we sense this is by waiting for the rapid to send back a ripple the ripple then tell us the position of the planet or moon and once we know the position we can teleport to that position and map that part of that solar system.
 

VISUAL EXERCISE
STEP ONE
Get comfortable and relax.

STEP TWO
Now I want you to see your visual body in front of your physical body and prepare your visual body for interstellar travel by placing an atmospheric bubble shield and a invisibility shield around your visual body. Then in your own time teleport your visual body out to your desired destination.

STEP THREE
Now I want you to construct a illusional energy rapid around the center of your visual body.

STEP FOUR
Now the difference between the ring of power and the detection ring is the ring of power draws energy and the detection ring is designed to detect a planet or moon in whatever solar system or star system that you may be visiting in your travels. So telepathically instruct the detection ring to expand and seek out any planets or moons in that solar system or star system.

STEP FIVE
As the interstellar detection rapid expands instruct the energy rapid to make a energy wave if it hits an planetary object as it expands out.

STEP SIX
Now if the energy rapid activates a wave teleport your visual body out to the point were the energy wave happened in that solar system or star system and see if there is a planet or moon in that area.

STEP SEVEN
When you have finished mapping that solar system or star system  draw the energy ring back into your hands in the usual way.

STEP EIGHT
Then teleport your visual body back to earth in front of your physical body and open your eyes and write down all of your finding.

Added On 28/01/2006

Planetary Composition Rapid

Planetary Detection Rapid

Programming A Planetary Detection Rapid

Once you have created an interstellar planetary detection rapid. Then the next step is to program it. Without opening your eyes project the energy rapid around your body so that the energy rapid is passing through your hands, then speak to your energy rapid Tell it to change colour when it passes through a planetary body that meets the composition of a planet on the list below, make sure you program each object type and colour. The Rapid should look like the one above when it is actived in interstellar space. For checking this technology try the new detection rapid on some of the destinations on the side bar.
 
 

Planetary Composition Chart

Colour Chart
Object Type
Rose
Ammonia Cloud Jovian, Eccentric 
Dark Blue
Water Cloud Jovian 
Light Blue
Water Cloud Jovian, Eccentric 
Orange
Jovian 
Platinum
Sulfurous Cloud Jovian, Eccentric 
Gold
Jupiter-twin 
Indigo
Cloudy Hot Jupiter 
Purple
Clarified Jovian, Eccentric
Red 
Hot Super Earth 
Light Green
Earth Like
Yellow
Clarified Jovian
Maroon
Dark Hot Jupiter 
Pink
Clarified Neptunian 
White
Extra galactic Planet 
Silver
Pulsar Planet 
Dark Green
Oceanic Planet 
Brown
Brown Dwarf 

Planetary Comparisons

Planetary Detection Rapid

Pulsars were first discovered in late 1967 by graduate student Jocelyn Bell Burnell as radio sources that blink on and off at a constant frequency. Now we observe the brightest ones at almost every wavelength of light. Pulsars are spinning neutron stars that have jets of particles moving almost at the speed of light streaming out above their magnetic poles. These jets produce very powerful beams of light. For a similar reason that "true north" and "magnetic north" are different on Earth, the magnetic and rotational axes of a pulsar are also misaligned. Therefore, the beams of light from the jets sweep around as the pulsar rotates, just as the spotlight in a lighthouse does. Like a ship in the ocean that sees only regular flashes of light, we see pulsars turn on and off as the beam sweeps over the Earth. Neutron stars for which we see such pulses are called "pulsars", or sometimes "spin-powered pulsars," indicating that the source of energy is the rotation of the neutron star.

Planetary Detection Rapid

Pulsar Planetary Detection Rapid

Pulsar planetary detection rapids are used to detect planetary bodies in planetary nebulas and other star clusters in deep space. the energy rapid is projected by the interstellar traveler with the intent of detecting planetary bodies orbiting distant stars.

Galaxies are large systems of stars and interstellar matter, typically containing several million to some trillion stars, of masses between several million and several trillion times that of our Sun, of an extension of a few thousands to several 100,000s light years, typically separated by millions of light years distance. They come in a variety of flavors: Spiral, lenticular, elliptical and irregular. Besides simple stars, they typically contain various types of star clusters and nebulae.

We live in a giant spiral galaxy, the Milky Way Galaxy, of 100,000 light years diameter and a mass of roughly a trillion solar masses. The nearest dwarf galaxies, stellites of the Milky Way, are only a few 100,000 light years distant, while the nearest giant neighbor, the Andromeda Galaxy, also a spiral, is about 2-3 million light years distant.

Planetary Detection Rapid

Galaxy Planetary Detection Rapid

Galaxy planetary detection rapids are used to dect planetary bodies Orbiting around Galatic core of a galaxy clusters of stars in a galaxy can contain many different planetary bodies. the energy rapid is porjected by the interstellar traveler with the intent of detecting planetary bodies orbiting around a star much like our sun in a galaxy.

Spiral Galaxies

Spiral galaxies usually consist of two major components: A flat, large disk which often contains a lot of interstellar matter (visible sometimes as reddish diffuse emission nebulae, or as dark dust clouds) and young (open) star clusters and associations, which have emerged from them (recognizable from the blueish light of their hottest, short-living, most massive stars), often arranged in conspicuous and striking spiral patterns and/or bar structures, and an ellipsoidally formed bulge component, consisting of an old stellar population without interstellar matter, and often associated with globular clusters. The young stars in the disk are classified as stellar population I, the old bulge stars as population II. The luminosity and mass relation of these components seem to vary in a wide range, giving rise to a classification scheme. The pattern structures in the disk are most probably transient phenomena only, caused by gravitational interaction with neighboring galaxies.
Our sun is one of several 100 billion stars in a spiral galaxy, the Milky Way.

Lenticular>

These are, in short, "spiral galaxies without spiral structure", i.e. smooth disk galaxies, where stellar formation has stopped long ago, because the interstellar matter was used up. Therefore, they consist of old population II stars only, or at least chiefly. From their appearance and stellar contents, they can often hardly be distinguished from ellipticals observationally.

Elliptical

Elliptical galaxies are actually of ellipsoidal shape, and it is now quite safe from observation that they are usually triaxial (cosmic footballs, as Paul Murdin, David Allen, and David Malin put it). They have little or no global angular momentum, i.e. do not rotate as a whole (of course, the stars still orbit the centers of these galaxies, but the orbits are statistically oriented so that only little net orbital angular momentum sums up). Normally, elliptical galaxies contain very little or no interstellar matter, and consist of old population II stars only: They appear like luminous bulges of spirals, without a disk component.
However, for some ellipticals, small disk components have been discovered, so that they may be representatives of one end of a common scheme of galaxy forms which includes the disk galaxies.

Irregular>

Often due to distortion by the gravitation of their intergalactic neighbors, these galaxies do not fit well into the scheme of disks and ellipsoids, but exhibit peculiar shapes. A subclass of distorted disks is however frequently occuring.

 As the 1990s began, the only planetary star system known was our own Solar System. The first extra-solar star system was discovered orbiting a pulsar in 1991. Slight changes in the precise arrival times of the pulses from the central small dense neutron star gave evidence of orbiting planets. By mid-decade Jupiter-like planets around Sun-like stars were being found by a slight wobble detected in the motion of these stars. Pictured above is an artist's sketch of a planet discovered orbiting HD217107. As the decade comes to a close, over two dozen planetary star systems have been identified, one recently confirmed by the detection of a slight eclipse by the planet itself. An unambiguous discovery of Sun-like star systems containing Earth-like planets still remains a goal.

Planetary Detection Rapid

Star Planetary Detection Rapid

Star planetary detection rapids are used to detect planetary bodies that are orbiting around stars and other star clusters in deep space. the energy rapid is projected by the interstellar traveler with the intent of detecting planetary bodies orbiting distant stars.

Milky Way Galaxy

Planetary Detection RapidThe Milky Way is the galaxy which is the home of our Solar System together with at least 200 billion other stars (more recent estimates have given numbers around 400 billion) and their planets, and thousands of clusters and nebulae, including at least almost all objects of Messier's catalog which are not galaxies on their own (one might consider two globular clusters as possible exceptions, as probably they are just being, or have recently been, incorporated or imported into our Galaxy from dwarf galaxies which are currently in close encounters with the Milky Way.

The spiral arms of our Milky Way contain interstellar matter, diffuse nebulae, and young stars and open star clusters emerging from this matter. On the other hand, the bulge component consists of old stars and contains the globular star clusters; our galaxy has probably about 200 globulars, of which we know about 150. These globular clusters are strongly concentrated toward the Galactic Center: From their apparent distribution in the sky, Harlow Shapley has concluded that this center of the Milky Way lies at a considerable distance (which he overestimated by factors) in the direction of Sagittarius and not rather close to us, as had been thought previously.

Our solar system is thus situated within the outer regions of this galaxy, well within the disk and only about 20 light years above the equatorial symmetry plane but about 28,000 light years from the Galactic Center. Therefore, the Milky Way shows up as luminous band spanning all around the sky along this symmetry plane, which is also called the "Galactic Equator". Its center lies in the direction of the constellation Sagittarius, but very close to the border of both neighbor constellations Scorpius and Ophiuchus


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