Asteroids are made up of the same materials as Earth, and other planets, but in different quantities. Our planet’s gravitational pull has resulted in most of its iron-loving materials being sucked to the core billions of years ago. This left the crust almost completely depleted of these elements. Without a gravitational pull, the metals on asteroids have remained close to the surface. Over millions of years, asteroid impacts deposited metals on the Earth’s crust. These have since been extracted in large quantities, and the resources are once again running out.
Space corporations are currently looking into the possibility of asteroid mining which would consist of taking metals, and other useful materials, from the surface of the asteroids. These extractions can be used in space, or taken back to Earth, and include: water and oxygen to sustain astronauts while in space, gold and palladium to send back to Earth, iron and titanium for space construction and hydrogen and ammonia as rocket propellant. The asteroids that are closest to our planet, would be the first targets. Investors believe that once asteroid mining has been perfected, it will become a trillion dollar industry.
There are three types of asteroids that are being considered for mining:
C- type – These asteroids have an abundance of water, and would be ideal places to refill astronaut supplies during space exploration. The option of stopping for water would greatly reduce mission costs. In addition, they also have organic carbon which would allow food growth.
S-Type – The surface of these asteroids is full of numerous metals, such as cobalt, nickel, gold and platinum.
M-Type – A source of up to ten times the amount of metal on S-type Asteroids.
Scientists have come up with three ways in which asteroid mining can be performed: mining the asteroid and bring the raw materials back to Earth, processing the materials before leaving to produce propellant to fuel the return trip or transporting the asteroid to a safe orbit around the moon, or our planet, where it would then be studied and mined.
A leader in space exploration, NASA has been researching asteroid mining for many years. They have already launched OSIRIS-REx on September 8, 2016, to facilitate the study of asteroid 101955 Bennu. The spacecraft will return to Earth with a sample of its surface in 2023, so that it can be studied in detail. If OSIRIS-REx is successful it will be the first mission that has brought an asteroid sample back to Earth.
NASA is also currently working on a mission called the Asteroid Redirect Mission (ARM). The aim of this project is for a spacecraft to use robotic arms and anchoring grippers which it will be fitted with, to retrieve a 4 metre boulder from a near-earth asteroid. The boulder will then be transported to a stable lunar orbit for analysis by robotic probes and future missions. ARM will be launched in December 2020.
The study was conducted by a team of researchers from Shinshu University. The method they proposed would involve transplanting stem cells into the heart, encouraging it to repair itself. Stem cell transplants have already been used to treat leukemia, lymphoma, Parkinson’s Disease and Alzheimer’s successfully. The process recommended by Shinshu has already been tried on primates, with good results. Some of the hearts with the transplanted cells began to beat irregularly, but there were no adverse effects of this and scientists are confident that the procedure will work well for humans.
After many years of research, Mayo Clinic has also developed a procedure that has allowed the successful transplant of stem cells into patients with heart disease. Their process involves harvesting these cells directly from the patient’s bone marrow, and then changing them into cardiac cells in a laboratory. These are then injected into the patient’s heart, where they will stimulate the growth of healthy tissue.

Matloff attempted to test and expand these theories, by locating astronomical objects that unexpectedly adjust their behavior in response to stimuli. This led to his study of Paranego’s Discontinuity, which is a theory that demonstrates where cooler stars orbit our galaxy at a faster pace than hotter ones. Science has attributed this phenomena to the stars’ interactions with gas clouds. Matloff noted that these changes only occurred in stars that were cool enough to have molecules in their atmosphere and, therefore, a more complex chemical composition. He also noted that some stars emit jets that only point in a single direction, which caused them to move in a different way.
The size of the star determines the amount of energy that it can produce. Larger ones have more heat and pressure, and can fuse heavier elements in a process known as nuclear fusion. Our sun, and other stars that are similar in size, produces energy in the core when Hydrogen atoms are converted into Helium. During this fusion, matter is released from the nuclei and converted to photons. It is estimated that 620 million metric tons are fused in our sun’s core in a single second. This is enough energy to power a large city for approximately 100 years!
This energy is essential to the survival of life on our planet. Once it arrives at our atmosphere, much of the UV radiation produced during nuclear fusion is filtered by The Ozone Layer, making it less harmful to our organisms. The benefits of the sun’s rays to our planet, are extensive and include warming our seas, generating weather patterns and providing energy for plants that in turn create food and oxygen for other lifeforms. Scientists have observed where the sun’s nuclear fusion patterns are relatively stable, even though there have been slight irregularities throughout many years. They are unsure of what has caused these short-lived changes, or the effects that the more drastic ones may have on our planet since the sun affects the way in which the entire Solar System functions.
Scientists from The University of Massachusetts Medical School have published an article in Nature, which states the possibility of decreasing the spread of HIV using cells which occur naturally in our bodies. Ironically, these are the same cells which the virus attacks. HIV breaks down the immune system by infecting and destroying CD4 positive ‘helper’ T-cells.
The researchers found that there are proteins in the T-cells in our immune system which naturally fight HIV. SERINC5 and SERINC3, two host cell proteins, are able to stifle HIV-1 by greater than 100-fold. The HIV-1 genome has nine genes which can be replicated in the host cell, which then produce virions (the infectious part of the virus). They begin a cycle of infection by looking for new cells to infect. One of these, NEF (which is a key part in the development of AIDS) helps the process by blocking the SERINC proteins, so that they are unable to reach the cell’s surface. This means that they will no longer become a part of the newly formed virions. Developing a drug to restrict NEFs would allow the system to fight HIV, as the virions would then include SERINC3 and SERINC5 making them unable to infect new cells. This process could then be applied to other infectious viruses with NEF proteins.