NSCI 314 LIFE IN THE COSMOS 3 – STARS AND THEIR EVOLUTION (CONTINUED) AND BASIC PROPERTIES OF LIFE Dr. Karen Kolehmainen Department of Physics CSUSB COURSE WEBPAGE:

REVIEW OF STAR FORMATION FORMED FROM A NEBULA (DENSER PART OF THE INTERSTELLAR MEDIUM) NEBULA CONTRACTS DUE TO GRAVITY SPINS FASTER AND FLATTENS INTO A DISK AS IT CONTRACTS GETS HOTTER, EVENTUALLY HOT ENOUGH FOR NUCLEAR FUSION (H TO He) TO BEGIN IN THE CENTER NOW IT IS A MAIN SEQUENCE STAR PLANETS AND SMALLER OBJECTS FORM FROM MATERIAL LEFT OVER

HIGH TEMPERATURE IS NECESSARY FOR NUCLEAR FUSION. THE NUCLEI MUST BE MOVING FAST ENOUGH TO COLLIDE DESPITE THEIR ELECTRICAL REPULSION. IN THE CORE OF A MAIN SEQUENCE STAR, TEMPERATURE IS ABOUT 15 MILLION K (27 MILLION o F). HYDROGEN NUCLEI (PROTONS) FUSE TO FORM HELIUM. FOUR 1 H (PROTONS) FUSE TO ONE 4 He + ENERGY. TWO OF THE PROTONS ARE CONVERTED TO NEUTRONS. WHERE DOES THE ENERGY COME FROM? ONE 4 He IS 0.7% LIGHTER THAN FOUR 1 H COMBINED. THE LOST MASS IS CONVERTED TO ENERGY. E = m c 2 ENERGY = MASS x (SPEED OF LIGHT) ² NUCLEAR REACTIONS IN MAIN SEQUENCE STARS

THE SUN CONVERTS 4 BILLION kg OF MATTER INTO ENERGY EACH SECOND. THE SUN HAS SUFFICIENT HYDROGEN TO DO THIS FOR 100 BILLION YEARS, BUT WILL STOP AFTER ABOUT 10 BILLION YEARS BECAUSE ONLY THE CORE UNDERGOES FUSION. (THE OUTER PARTS OF THE STAR AREN’T HOT ENOUGH FOR FUSION.) WHEN HYDROGEN IN THE CORE RUNS OUT, THIS MARKS THE END OF THE MAIN SEQUENCE LIFETIME. THE MORE MASSIVE THE STAR, THE SHORTER THE MAIN SEQUENCE LIFETIME. EVEN THOUGH THERE IS MORE HYDROGEN TO FUSE, FUSION PROCEEDS SO MUCH MORE RAPIDLY (BECAUSE IT IS HOTTER) THAT THE HYDROGEN IN THE CENTER DOESN’T LAST AS LONG. NUCLEAR REACTIONS IN MAIN SEQUENCE STARS

MAIN SEQUENCE STARS ALL PROPERTIES OF A MAIN SEQUENCE STAR DEPEND ON ITS MASS. –MORE MASSIVE STARS ARE LARGER. –MORE MASSIVE STARS ARE HOTTER. –MORE MASSIVE STARS ARE BLUER. –MORE MASSIVE STARS ARE BRIGHTER. –MORE MASSIVE STARS HAVE SHORTER LIFETIMES. EVEN THOUGH THEY HAVE MORE NUCLEAR FUEL, THEY USE IT UP MORE QUICKLY BECAUSE OF THEIR HIGHER TEMPERATURES.

Brightness (Sun = 1) Spectral Type Number of Stars in MW Percent of Total 100, OBAFGKMOBAFGKM 5 million 10 million 500 million 1 billion 10 billion 100 billion 1 trillion 80, million 2.4 billion 12 billion 28 billion 60 billion 290 billion % 0.09 % 0.6 % 3 % 7 % 15 % 73 % Lifetime (Years) PROPERTIES OF MAIN SEQUENCE STARS

AT THE END OF THE MAIN SEQUENCE LIFETIME… THE OUTER PART OF THE STAR EXPANDS (BY UP TO 200 TIMES), BRIGHTENS (BY UP TO 100 TIMES), AND COOLS TO 3,000 K. THE STAR BECOMES A RED GIANT. IN MASSIVE STARS, A SECOND STAGE OF EXPANSION AND COOLING PRODUCES A SUPERGIANT. MEANWHILE, THE CORE CONTRACTS AND HEATS UP UNTIL HELIUM BEGINS TO FUSE TO FORM CARBON AND HEAVIER ELEMENTS. THE STAR GOES THROUGH OCCASIONAL EPISODES OF INSTABILITY, WITH RAPID OSCILLATIONS IN SIZE, TEMPERATURE, AND BRIGHTNESS.

He FUSES INTO CARBON, NITROGEN AND OXYGEN + ENERGY. IN LOW MASS STARS, FUSION STOPS HERE BECAUSE IT NEVER GETS HOT ENOUGH TO FUSE C, N, AND O TO EVEN HEAVIER ELEMENTS. IN MASSIVE STARS, CARBON FUSES TO FORM HEAVIER ELEMENTS, WHICH AGAIN FUSE TO FORM EVEN HEAVIER ELEMENTS, EVENTUALLY RESULTING IN IRON. AT EACH STEP, ENERGY IS PRODUCED. FUSION OF IRON TO EVEN HEAVIER ELEMENTS WOULD REQUIRE ENERGY AS AN INPUT INSTEAD OF RELEASING ENERGY. (THE NUCLEUS THAT WOULD RESULT FROM FUSION IS HEAVIER THAN THE NUCLEI THAT WOULD FUSE TO FORM IT.) THIS ENERGY IS UNAVAILABLE, SO FUSION DOESN’T PROCEED BEYOND IRON, NO MATTER HOW MASSIVE THE STAR. NUCLEAR REACTIONS IN RED GIANTS AND SUPERGIANTS

LATE STAGES OF STELLAR EVOLUTION FOR SOLAR-TYPE (LOW MASS) STARS PLANETARY NEBULA: THE OUTER PART OF THE STAR IS EJECTED. THE EJECTED MATERIAL EXPANDS, COOLS, AND ENRICHES THE INTERSTELLAR MEDIUM WITH HEAVIER ELEMENTS (FUSION PRODUCTS). THE CORE OF STAR REMAINS IN THE CENTER OF THE NEBULA, AND BECOMES A … WHITE DWARF: CORE OF THE ORIGINAL STAR LEFT AFTER OUTER PARTS ARE EJECTED. IT SHRINKS TO ABOUT EARTH-SIZE, AND IS VERY DENSE. (A TEASPOONFUL OF WHITE DWARF MATERIAL WOULD WEIGH ABOUT A TON.) THERE IS NO MORE FUSION, SO THE WHITE DWARF COOLS AND DIMS (VERY, VERY SLOWLY) UNTIL EVENTUALLY IT BECOMES A … BLACK DWARF: NO MORE LIGHT EMITTED. STELLAR CORPSE IS A DENSE SOLID BALL OF CARBON, NITROGEN, AND OXYGEN. THE UNIVERSE ISN'T OLD ENOUGH FOR BLACK DWARFS TO HAVE FORMED YET.

LATE STAGES OF STELLAR EVOLUTION FOR MASSIVE STARS SUPERNOVA (TYPE II) – IRON CORE OF RED SUPERGIANT COLLAPSES UNTIL NUCLEI COLLIDE WITH EACH OTHER. – NUCLEI BOUNCE APART VIOLENTLY, PUSHING MATERIAL OUTWARD AND CAUSING STAR TO EXPLODE. – LOTS OF ENERGY IS RELEASED IN EXPLOSION, STAR BRIGHTENS ENORMOUSLY. – ENERGY OF EXPLOSION CAUSES FUSION OF HEAVY ELEMENTS (EVEN HEAVIER THAN IRON). – EJECTED MATERIAL FORMS A SUPERNOVA REMNANT, WHICH EXPANDS AND ADDS MATERIAL (ENRICHED IN HEAVY ELEMENTS) TO THE INTERSTELLAR MEDIUM. NEUTRON STAR OR BLACK HOLE: CORE OF ORIGINAL STAR LEFT OVER AFTER THE SUPERNOVA EXPLOSION, EXTREMELY DENSE

“BEFORE AND AFTER” PICTURES OF A SUPERNOVA

NEUTRON STAR BALL OF NEUTRONS (LIKE ONE BIG NUCLEUS) MASS BETWEEN ABOUT 1.4 AND 3 SOLAR MASSES RADIUS ABOUT 10 km VERY HIGH DENSITY – ONE TEASPOONFUL OF NEUTRON STAR MATERIAL WOULD WEIGH A BILLION TONS MANY NEUTRON STARS EMIT PULSES OF RADIO WAVES AND OTHER ELECTROMAGNETIC RADIATION, AND ARE OBSERVED AS PULSARS

BLACK HOLE IF THE STELLAR CORE LEFT AFTER A SUPERNOVA IS SUFFICIENTLY MASSIVE (MORE THAN ABOUT 3 SOLAR MASSES), IT COLLAPSES TO FORM A BLACK HOLE EVEN HIGHER DENSITY THAN A NEUTRON STAR ESCAPE VELOCITY EXCEEDS THE SPEED OF LIGHT

ESCAPE VELOCITY SPEED NEEDED WHEN TAKING OFF FROM THE SURFACE OF A PLANET OR OTHER OBJECT IN ORDER TO ESCAPE THE OBJECT’S GRAVITY (TECHNICALLY, TO ESCAPE TO AN INFINITE DISTANCE AWAY, SLOWING TO ZERO SPEED IN THE PROCESS). EARTH'S ESCAPE VELOCITY IS 11 km/s. THE MORE MASSIVE THE OBJECT YOU'RE ESCAPING FROM, THE LARGER THE ESCAPE VELOCITY. THE SMALLER THE RADIUS OF THE OBJECT YOU'RE ESCAPING FROM, THE LARGER THE ESCAPE VELOCITY. THEREFORE, A MASSIVE BUT SMALL OBJECT (i.e., A DENSE OBJECT) HAS A LARGE ESCAPE VELOCITY.

BLACK HOLE ESCAPE VELOCITY EXCEEDS THE SPEED OF LIGHT. THEREFORE NOTHING CAN ESCAPE, NOT EVEN LIGHT. AN “EVENT HORIZON” SEALS OFF THE INTERIOR FROM THE REST OF THE UNIVERSE. THE EVENT HORIZON HAS A RADIUS OF SEVERAL km FOR A STELLAR MASS BLACK HOLE. MATTER INSIDE EVENT HORIZON PROBABLY CONTRACTS TO A “SINGULARITY” – INFINITE DENSITY! CAN SOMETIMES BE DETECTED VIA GRAVITATIONAL EFFECTS ON OTHER OBJECTS (E.G., IN A DOUBLE STAR SYSTEM) AND/OR VIA X-RAYS EMITTED BY MATTER FALLING IN. IN ADDITION TO STELLAR-MASS BLACK HOLES FORMED AT END OF LIVES OF MASSIVE STARS, LARGER BLACK HOLES EXIST IN THE CENTER OF MOST GALAXIES (INCLUDING THE MILKY WAY).

A CLOSED SYSTEM AND ITS ENVIRONMENT CLOSED SYSTEM MATTER ENERGY MATTER ENERGY

AN OPEN SYSTEM AND ITS ENVIRONMENT OPEN SYSTEM MATTER ENERGY WASTE ENERGY WASTE MATTER

ENTROPY AND ORDER ENTROPY: A MEASURE OF THE DISORDER IN A SYSTEM – LOW ENTROPY = HIGHLY ORDERED – HIGH ENTROPY = VERY DISORDERED OR MESSY SECOND LAW OF THERMODYNAMICS: – IN ANY CLOSED SYSTEM (MEANING THAT NOTHING ENTERS OR LEAVES), NO PROCESS CAN OCCUR IN WHICH THE SYSTEM'S ENTROPY DECREASES. IN OTHER WORDS, A CLOSED SYSTEM CAN'T BECOME MORE ORDERED (LESS MESSY) AS TIME GOES ON. – THEREFORE, THE AMOUNT OF DISORDER IN A CLOSED SYSTEM EITHER INCREASES WITH TIME OR IT DOESN’T CHANGE WITH TIME. USUALLY, THE ENTROPY INCREASES WITH TIME, i.e., A CLOSED SYSTEM GETS MESSIER AS TIME GOES ON.

ENTROPY AND ORDER SECOND LAW OF THERMODYNAMICS: IN ANY CLOSED SYSTEM, NO PROCESS CAN OCCUR IN WHICH THE ENTROPY DECREASES WITH TIME, i.e., A CLOSED SYSTEM CANNOT BECOME MORE ORDERED WITH TIME. WHAT ABOUT THE ENTROPY OF AN OPEN SYSTEM? AN OPEN SYSTEM INTERACTS WITH ITS ENVIRONMENT. IF WE INCLUDE THE ENVIRONMENT AS PART OF THE SYSTEM (INSTEAD OF SOMETHING OUTSIDE OF THE SYSTEM), WE NOW HAVE A CLOSED SYSTEM, AND ITS TOTAL ENTROPY CAN'T DECREASE WITH TIME. HOWEVER, THE ENTROPY OF THE ORIGINAL OPEN SYSTEM CAN DECREASE, AS LONG AS THE ENTROPY OF ITS ENVIRONMENT INCREASES BY AN EVEN LARGER AMOUNT. LIFE: ENTROPY DECREASES WITHIN AN ORGANISM AS RAW MATERIALS ARE REARRANGED IN HIGHLY ORDERED WAYS. HOWEVER, THE ORGANISM IS AN OPEN SYSTEM, AND THE ENTROPY OF ITS ENVIRONMENT INCREASES.

LIFE AND ITS ENVIRONMENT ORGANISM ENTROPY DECREASES MATTER ENERGY WASTE MATTER WASTE ENERGY ENVIRONMENT ENTROPY INCREASES

WHAT IS LIFE? HARD TO DEFINE, BUT LET'S LIST SOME OF ITS PROPERTIES. NECESSARY PROPERTIES: – USES ENERGY – INTERACTS WITH ITS ENVIRONMENT – MAINTAINS A LOW ENTROPY (HIGH DEGREE OR ORDER OR COMPLEXITY) INTERNALLY LIKELY (BUT MAYBE NOT NECESSARY) PROPERTIES: – GROWS AND DEVELOPS – REPRODUCES – MUTATES AND EVOLVES

REQUIREMENTS FOR LIFE MATTER: PRODUCED IN BIG BANG (H & He) AND STARS (HEAVIER ELEMENTS) ARE CERTAIN ELEMENTS NEEDED? STABLE ENERGY SOURCE: LOW MASS MAIN SEQUENCE STARS (OR SOMETHING ELSE?) PROTECTED ENVIRONMENT: PLANETARY OR LUNAR SURFACES PLANETARY OR LUNAR INTERIORS THICK PLANETARY OR LUNAR ATMOSPHERES CHEMICAL SOLVENT (LIQUID): WATER (OR SOMETHING ELSE?) APPROPRIATE TEMPERATURE RANGE: NEEDED TO KEEP THE SOLVENT LIQUID (APPROXIMATELY 0 TO 100 o C IF WATER IS THE LIQUID SOLVENT) IF IT’S TOO HOT, COMPLEX STRUCTURES ARE BROKEN APART IF IT’S TOO COLD, INTERACTIONS ARE TOO SLOW

Sun Earth Earth’s Crust Hydrogen Helium Oxygen Carbon Neon Nitrogen Magnesium Silicon Iron Sulfur Argon Aluminum Calcium Sodium Nickel Chromium Phosphorus 90.99% Oxygen Iron Silicon Magnesium Sulfur Nickel Aluminum Calcium Sodium Chromium Phosphorus 50% Oxygen Silicon Aluminum Iron Calcium Sodium Potassium Magnesium Titanium Hydrogen Phosphorus Manganese Fluorine Strontium Sulfur 47%

Earth’s Atmosphere Bacteria Human Beings Nitrogen Oxygen Argon Carbon** Neon Helium 78% Hydrogen Oxygen Carbon Nitrogen Phosphorus Sulfur 63% Hydrogen Oxygen Carbon Nitrogen Calcium Phosphorus Sulfur 61%

BOTTOM LINE: THE ELEMENTS THAT MAKE UP TERRESTRIAL LIVING ORGANISMS ARE VERY COMMON IN STARS AND IN THE INTERSTELLAR MATERIAL FROM WHICH STARS AND PLANETS ARE FORMED. IN LIVING THINGS, THE ATOMS OF THESE ELEMENTS ARE ORGANIZED IN ORGANIC MOLECULES, MANY OF WHICH ARE LARGE AND COMPLEX.

ORGANIC MOLECULES MOLECULE: A COMBINATION OF TWO OR MORE ATOMS EXAMPLES: H 2 O CO 2 CH 4 NH 3 H 2 N 2 O 2 C 2 H 5 O 2 N ORGANIC MOLECULE: A MOLECULE COMPOSED OF CARBON AND HYDROGEN ATOMS (AND OFTEN OTHER ELEMENTS ALSO) EXAMPLES: CH 4 C 2 H 5 O 2 N MONOMER: A SIMPLE ORGANIC MOLECULE SUCH AS AN AMINO ACID, SIMPLE SUGAR, FATTY ACID, OR GENETIC BASE POLYMER: A LARGE ORGANIC MOLECULE COMPOSED OF A CHAIN OF REPEATING MONOMERS

EXAMPLES OF POLYMERS CARBOHYDRATES: STARCHES, CELLULOSE, SUCROSE. MONOMERS: SIMPLE SUGARS, GLUCOSE LIPIDS: FATS, CHOLESTEROL, HORMONES, CELLULAR MEMBRANES. MONOMERS: FATTY ACIDS NUCLEIC ACIDS: DEOXYRIBONUCLEIC ACID (DNA) & RIBONUCLEIC ACID (RNA). MONOMERS: GENETIC BASES PROTEINS: STRUCTURAL PROTEINS FOR BONE, ORGANS, TISSUE, AND MEMBRANES; ENZYMES, CHEMICAL SENSORS AND TRANSPORTERS. MONOMERS: AMINO ACIDS NEXT TIME: LET’S EXAMINE NUCLEIC ACIDS AND PROTEINS IN MORE DETAIL.