Claudia Albers - The Planet X Report 2017: Photographic Evidence

Chapter 1

Introduction

There is mounting evidence for Stellar Cores in the Suns Corona. These objects seem to have been mentioned in the 1980s and Dr. Robert Harrington was one of the first astronomers to search for these objects in the 1990s. He called them Planet X and this is the reason why they are called Planet X in this book. The Planet X system seems to be made up of a large number of Stellar Cores. These Stellar Cores are changing the Sun and affecting our planet and yet the powers that be do not want the public to know the truth. This book is an attempt to remedy that. The first three chapters contain an introduction to Planet X Stellar Cores and what they reveal about the Sun and the Universe. The next nine chapter contain what I believe are the best and most important articles I have written on this subject.

Dr. Claudia Albers

Planet X Physicist

Chapter 2

Introduction to Stellar Cores

Stellar Cores are solid objects observed in the Suns corona. The images below are from 2001 and are therefore some of the first images available in which we can observe these objects. One of the objects is observed eclipsing the sun and several can be seen at the bottom edge of the images. The round outline visible on the bottom right corner of the middle image, indicates the presence of one of these Stellar Cores, another is present in the left bottom corner of the third image. Both of these objects are dark and partly covered in plasma from the Suns corona.

Figure 1.1 . Yohkoh spacecraft x-ray images of the Sun from December 14 th 2001 at 14:19, 20:50 and 20:58 (UTC). These are the last images available at Helioviewer.org from this telescope. The last two images show an object which emits radiation homogeneously across its surface, and therefore a star, but is not nearly as bright as the Sun moving in front of the spacecrafts detectors.

Yohkoh, which in Japanese means Sunbeam. It was a solar observatory spacecraft launched by Japan and operated in collaboration with NASA and the UKs space agency. It was launched in 1991 and was also known as Solar A. The images we see in figure 1.1 above are from its soft (low energy) x-ray telescope. The images show an object eclipsing the Sun which is obviously emitting x-rays. If the object had been a planet it would look completely black, in the image, as planets do not emit x-rays. This means that the object is most likely to be a star.

From the circular outline of the Stellar core seen in the middle image in figure 1.1 we can deduce that the object is between one third and half the size of the Sun and we can do this because the object is obviously enveloped in coronal plasma and in the Suns corona and therefore close enough to the Sun to make it possible to make a direct size comparison with the Sun.

These objects have to be stars, as only stars can survive the very hot environment in the Suns corona. They are also solid objects and must be extremely dense in order not to melt or sublimate at temperatures of millions of degrees kelvin. The Suns core is believed to have a density of 150 g/cm . And so the Stellar Cores will most likely have a comparable density to the Suns core. The Stellar Cores are cores of stars that were once main sequence stars but have gone through an ageing process that saw them go through the red giant and white dwarf phases. During this process they lose their outer layers of ionizing material, and eventually the stars core is exposed, as we observe for the Blue Stellar Core, shown below. The object is obviously solid with only a small amount of material clinging to its surface. This material is what is left of its original ionizing material which the star starts losing when it enters the red giant phase. The Blue Stellar Core has been left with a very small amount of ionizing material clinging to the surface of the stars solid core. The star will still ionize and boil off this material, turn into gaseous plasma, which it then exchanges with the Sun. The plasma connection between the Stellar Core and the Sun is clearly visible in the image as a thin white line between the Suns corona and the pink gaseous plasma accumulating below the Stellar Core.

Figure 1.2 Telescopic photograph of the Blue Stellar Core in the Suns corona. Grooves on the surface of the object show that it is solid. The fact that it has not melted, when immersed in the Suns corona, which is at a temperature of millions of degrees kelvin, shows that it is in an extremely dense state of matter, as expected of the core of a star. The magenta colored gaseous plasma may indicate the presence of argon which gives off magenta light when ionized.

The fact that Stellar Cores are basically exposed cores of stars that must have gone through a process through which they have lost their many layers of star material, which I like to call ionizing material, as this is the material that a star ionizes into a plasma and uses to emit light. We know this process as the ageing process stars go through when they go through the red giant and white dwarf phases. So it is not surprising that these stars have some similarities to white dwarfs and this is the reason why they may sometimes be referred to in this book as Brown Dwarf stars. Another term that may sometimes be used is Stellar Remnant, a fitting term since these objects seem to be the remnant of what was once living and light emitting main sequence stars, which have aged to the point that they no longer are able to emit light and may then be described as dead stars. Some Brown Dwarf stars or Stellar Cores have not aged yet to the point where just about all of their ionizing material is gone as with the Blue Stellar Core. Some still have a complete toroidal shaped ionizing envelope left over from the white dwarf phase. One such Stellar Core can be seen below to have a cloud like disk shaped structure around it. This structure is its ionizing envelope.

Figure 1.3 . Enhanced telescopic photograph of the Blue Stellar Core, from July 26 th 2017, showing that the Suns corona has enveloped the object. This indicates that the object is magnetically connected to the Sun and is attracting the Suns plasma. A smaller disk shaped Stellar Core is observed below the Blue Stellar Core. The object also has coronal plasma draped along its edges but most of the object is dark. Its shape is similar to what white dwarfs are known to have.

Some of the characteristics that Stellar Cores are known to have in common with white dwarfs are:

• They have gaseous envelopes (see figure 1) [1].
• They are able to draw plasma from main sequence stars (see figure 2) [1,2];
• They are able to have nova outbursts (see figure 3) [1,2].
• They have very high magnetic fields (see figure 3) [1].