How Does Life Come From Randomness?
http://edu-observatory.org/olli/42/Week3.html



How Does Life Come From Randomness?  (2 min)
  Kaplan_Life_Randomness.mp4

  



Feynman Lectures On Physics
  https://www.feynmanlectures.caltech.edu   
Feynman Lecture No. 1 - Atoms in Motion
  https://www.feynmanlectures.caltech.edu/I_01.html   
 
  Attractive intermolecular forces are categorized into the 
  following types:
    o Hydrogen bonding
    o Ion-dipole forces and ion-induced dipole forces
    o Van der Waals forces

  Two important principles:
    1. Evaporation: Cools the Water ==> Warms the Atmosphere
    2. No evaporation takes place when the relative humidity
       of the air is 100 percent (saturated)
  
  






Energy Sources When stars form, gravitational collapse heats the shrinking cloud of gas and dust to a high enough temperature (15 million Kelvin in the case of our Sun), that hydrogen nuclei (protons) can overcome their repulsive Coulomb Force and collide. By the weak interaction in quantum mechanics, one of the protons can be converted to a neutron, a positron, and a bit of energy, in the form of an escaping neutrino. We detect the solar neutrinos here on earth and measure their energy. The majority of the energy produced in stars like our sun comes from the gamma photons produced when an additional proton combines the proton-neutron pair to create light helium ³He nuclei. The energy sources for the earth are: 1. Radiation from the Sun (mostly visible light) 2. Internal heat from Radioactivity 3. Heat of formation (probably dissipated after 4.5 billion years) 4. Tidal Friction (from the gravitation of the Sun and Moon) 5. Impacts from solar system (asteroids, comets, meteoroids)

Essential elements of Life List of interstellar and circumstellar molecules (212+) https://en.wikipedia.org/wiki/List_of_interstellar_and_circumstellar_molecules https://www.chemistryworld.com/features/the-surprising-organic-chemistry-in-interstellar-space/4019144.article Thanks to advances in astronomical technology, we now know there are ever-evolving regions where densities of matter change, atomic clouds transform into molecular clouds that collapse under gravity giving birth to protostars. More than 260 different molecular species have now been detected in interstellar space, including alcohols, aldehydes, acids and amides and many other organic molecules – some familiar on Earth, some not stable here at all. All of the bases in DNA and RNA have now been found in meteorites https://www.sciencenews.org/article/all-of-the-bases-in-dna-and-rna-have-now-been-found-in-meteorites

Non-equilibrium thermodynamics https://en.wikipedia.org/wiki/Non-equilibrium_thermodynamics ORIGINS OF LIFE First Support for a Physics Theory of Life https://www.quantamagazine.org/first-support-for-a-physics-theory-of-life-20170726/ Non-equilibrium thermodynamics can help explain the creation of increasingly complex molecules by describing how systems far from equilibrium can evolve over time. In non-equilibrium conditions, external energy inputs drive systems away from thermodynamic equilibrium, allowing chemical reactions and processes that would not normally occur in equilibrium states. This can lead to the formation of complex structures, including molecules, through processes like self-organization, dissipative structures, and autocatalytic cycles. Such systems can absorb energy and maintain a state of dynamic flux, promoting reactions that create complexity. However, while non-equilibrium thermodynamics provides a framework, it doesn’t fully explain the emergence of molecular complexity, which also depends on factors such as specific chemical environments and reaction pathways.

Ribonucleic acid (RNA) A hairpin loop from a pre-mRNA. Highlighted are the nucleobases (green) and the ribose-phosphate backbone (blue). This is a single strand of RNA that folds back upon itself. A single strand of RNA that folds back upon itself forms what is called a secondary structure. This folding is significant for several reasons: The folding of RNA helps stabilize the molecule, enabling it to maintain its structure in the cellular environment. The formation of double-stranded regions through base pairing (typically between adenine and uracil, and between guanine and cytosine) can provide stability to the RNA molecule. Many RNAs, such as transfer RNA (tRNA) and ribosomal RNA (rRNA), rely on their secondary structures to perform their biological functions. For example, the cloverleaf structure of tRNA is crucial for its role in protein synthesis. The secondary structure of RNA can play a regulatory role in gene expression. Some regions of mRNA form secondary structures, such as hairpins or stem-loops, which can influence the efficiency of translation by affecting how ribosomes or regulatory proteins interact with the RNA. Some RNA molecules, known as ribozymes, have catalytic activity. The formation of specific secondary structures is essential for the proper alignment of the active sites required for these RNA molecules to perform enzymatic reactions. Many RNA viruses rely on specific secondary structures in their RNA genomes for replication, translation, and evasion of the host immune system. These folded RNA structures can serve as recognition sites for viral proteins or host factors. Overall, the ability of RNA to fold into specific secondary structures is crucial to its diverse roles in the cell, from catalysis to regulation and gene expression.

Science News Media The surprising organic chemistry in interstellar space https://www.chemistryworld.com/features/the-surprising-organic-chemistry-in-interstellar-space/4019144.article All of the bases in DNA and RNA have now been found in meteorites https://www.sciencenews.org/article/all-of-the-bases-in-dna-and-rna-have-now-been-found-in-meteorites Astronomers Discover Complex Carbon Molecules in Interstellar Space https://www.sciencealert.com/astronomers-discover-complex-carbon-molecules-in-interstellar-space First Look at Ryugu Asteroid Sample Reveals it is Organic-Rich https://www.nasa.gov/centers-and-facilities/goddard/first-look-at-ryugu-asteroid-sample-reveals-it-is-organic-rich/ Scientists Discover RNA Component Buried in The Dust of an Asteroid https://www.sciencealert.com/scientists-discover-rna-component-buried-in-the-dust-of-an-asteroid https://www.nature.com/articles/s41467-022-29612-x Never Before Detected – Organic Molecule Essential for Life Found in Interstellar Space https://scitechdaily.com/never-before-detected-organic-molecule-essential-for-life-found-in-interstellar-space/ https://www.nature.com/articles/s41467-023-36904-3 Nonequilibrium Processes https://sciurls.com/?btnG=sciurls&q=nonequilibrium Researchers verify relationship between rate of a nonequilibrium process and the rate at which it creates entropy https://phys.org/news/2022-02-rsearchers-relationship-nonequilibrium-entropy.html Latest Science (all sciences) http://edu-observatory.org/media/Science/index.html#LATEST ChatGPT https://chat.openai.com/chat DuckDuckGo
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