What Makes a Cancer Cell

by Sandra Ning, Terra Linda HS

Cancer is most commonly treated through radiation, surgery, and chemotherapy.

    While it could be considered cliché to compare cancer cells to supervillains, the similarities are undeniable. Supervillains are cunning, deeply rooted within their far-reaching schemes, and fearsome to the extreme. Cancer cells are just as sly, difficult to remove from the human body and terrifying to the afflicted and their loved ones. It’s not hard to visualize cancer cells as the shady criminal syndicate of the human body; their reach extends to the lungs, bones, tissue and bloodstream, and their tactics are ruthless. Make no mistake—cancer cells have long been antagonists to the scientists fighting for a cure and the patients fighting for their life.
    But when it comes down to the science of it, cancer cells differ from many classic villains in that they aren’t innately evil. Rather, cancer cells and their dangerous properties originate from chance mutations during the division of normal cells. Mutations explain a lot of strange phenomena, from unexpected eye colors to increased resistance to diseases. These unexpected changes in gene sequences can be harmless, or even beneficial. However, they have an equal chance of damaging DNA, mutating it in such a way that the cell distorts into fast-splicing cancer cells.
     Usually, mitosis—the process in which a cell divides—takes precautions against such mutations. “Checkpoints” during a cell’s growth period scan for identity-changing DNA mishaps, ensuring things are running as expected. If something is wrong, the cell will stop growing; if the damage to the DNA can’t be repaired, the cell will kill itself in a process called apoptosis. Through such self-sacrificing vigilance, cells that are mutated beyond repair never get the chance to multiply into a runaway number of damaged cells. But sometimes cell mutations go undetected, due to the sheer number of cells within the human body, with its trillions of constantly dividing cells, each with their own double-helix sequences and enzyme and lysosomes. In such a rush, a handful of mutations can slip by even the strict quality standards cells hold to themselves. Many of these mutations go undetected because they’re harmless to the identity of that cell—but some aren’t so benign.

Normal and cancer cell division. Most damaged cells die through apoptosis.

     When a cell with damaged DNA successfully slips by and divides, it creates the first two in a series of cells that will rapidly divide and spread incorrect DNA, beginning the first rapidfire stages of cancer. The speed of growth and division of cancer cells is unmatched, and unyielding; a cancer cell’s daunting ability to keep multiplying without ever dying, as normal cells do, is often referred to as ‘immortality’. This trait is due to two substances within the cell in particular: telomere and telomerase.
      Telomere is a repeating DNA sequence that essentially acts as a cap for the chromosome it’s on. The sequence acts as a buffer between valuable DNA sequences within the chromosome and the often messy process of dividing a cell. Without the telomere, the ends of the chromosome would lose important base pairs much like a rope fraying at the ends. The more a cell divides, the more telomere is lost in protecting the chromosome. Once all of the telomere is gone, the chromosome reaches “critical length” and no longer replicates. When this happens, the cell doesn’t divide and dies through apoptosis. The erosion of telomere thus measures the age of a cell, with long telomere sequences indicating young cells and short sequences indicating old ones.

The repeating TTGGGG sequence is telomere; the enzyme and RNA template belong to telomerase, which rebuilds worn-down telomere.

     To restore and keep the cycle of cells replicating in our body, telomerase is needed to extend the eroding telomeres. Telomerase is an enzyme made of proteins and RNA. As an enzyme, telomerase enables certain reactions that couldn’t happen without it—in this case, rebuilding and elongating telomeres to a longer sequence again. Telomerase is sparingly used in somatic, or body, cells, which comprise most of the human body. As a result, humans age without much interference from telomerase.
     While telomerase is rarely active in normal body cells, the enzyme becomes ten to twenty times more active in cancer cells. The abundance of telomerase gives cancer cells an endless supply of telomere, and with it, the ability to multiply indefinitely.
    In addition to ‘immortality,’ cancer cells have several additional unique properties that explain why finding a cure is proving so difficult. In addition to fast replication, cancer cells don’t undergo apoptosis easily; high levels of survivin, a protein, inhibits the usual method of cell death. Cancer cells need neither the physical space nor the same amount of nourishing chemicals, known as growth factors, that normal cells need. Instead, they pile freely on top of each other, and remain undeterred by a diet on growth factors. The clusters cancer cells often find themselves in form the lumps within the breasts and testes that doctors and outreach campaigns warn about. Despite their ability to clump, cancer cells have unfortunately high mobility, too. While normal cells anchor themselves onto neighboring cells, cancer cells can break away and travel through the body, infecting other organs. Their ability to invade and infect other areas is made possible through the ability to break through the lamina. The lamina is a noncellular shield that protects the tissues, organs and surfaces within the human body, deflecting normal cells with ease. Cancer cells don’t have the same limitation, and spread to different organs with relative ease.
     With its unique properties, cancer remains frustratingly difficult to cure. Treating cancer needs to somehow overcome the mobility and speed of replication cancer cells exhibit. Current treatments for cancer actually do better than that—the chemotherapy method of treatment uses the cancer cells’ speedy multiplication against it. Chemotherapy sends chemicals throughout the body that kill fast-replicating cells. Cancer cells are efficiently targeted and wiped out through this method, being some of the fasted replicating cells in the body.
     However, chemotherapy has serious faults in its accuracy; by targeting fast-replicating cells, chemotherapy hits hair and blood cells particularly hard. A broad swath of helpful cells get caught in the crossfire between chemotherapy and the cancer cells it’s meant to target. As a treatment for cancer, chemotherapy can cause hair loss, amongst other more painful side-effects.

Chemotherapy affects the fast-growing hair cells as well, which is why cancer patients’ hair often falls out.

     Other treatments are available, when cancer cells are concentrated in specific parts of the body. Radiation focuses on a single area, maybe one organ, to destroy cancer cells. When cancer cells are concentrated in a single area, forming a tumor, surgery can excise the infected part. Sometimes, a mixture of the three treatments are required to treat a patient.
     There is still no way to accurately target and eradicate cancer cells without collateral damage. For that reason, and for the growing number people with breast cancer, leukemia, and other forms of cancer, research for better treatment and ultimately a cure is incredibly important. Cancer is internal, deadly in its silent machinations and intimidating with its arsenal of lethal properties. It’s up to the bright minds and generous hearts of every scientist, doctor, donor and activist to combat, quite literally, the enemy within.

Interested in cancer cells and what scientists are doing to treat it? Come see Dr. Brad A. Stohr present “Why do Cancer Cells Grow Forever and Can we Stop Them?” Dr. Stohr will be presenting this Wednesday, April 17th, at the Marin Science Seminar. The Marin Science Seminar takes place during 7:30 to 8:30 p.m., in rm. 207 of Terra Linda High School. Come check out the Marin Science Seminar on our website and Facebook!

Sources:

Sandra Ning

The Birth of the Universe, through Today’s Telescopes

by Sandra Ning, Terra Linda HS

A nebula in the Large Magellanic Cloud. Though nebulae are often the focus of space appreciation in pop culture, the universe encompasses billions more phenomena.


     A story is typically told from the beginning, but oftentimes the universe is an exception. As a society, time is measured in days and nights, hours, minutes, and seconds. But even more so, time is apparent to us through the peachy sunrise of dawn, the angry grumbles of an empty stomach at noon, and the fatigue that settles with the darkness of night. It’s hard to imagine any of these things in relation to the universe, with its sleepless planets and nomadic asteroids, all swallowed up in an unimaginably large blanket of space. If the universe is a story, and all the galaxies, comets, and stars its characters, where does it all begin? 
     Luckily, scientists have already delved into the origins of the universe, and have resurfaced with new and exciting insights regarding these questions. Dr. Mary Barsony, an associate professor of physics and astronomy at SFSU, has kindly answered several questions regarding the birth of the universe, the elements, and how scientists are researching it all.

1. The Big Bang theory is the most widely-accepted theory for the creation of the universe. What kind of evidence have astrophysicists gathered to support this?


    a) Apart from the “immediate” neighborhood of our Milky Way Galaxy,
in any direction you look, the further away a galaxy is, the greater the shift
of its spectral lines towards longer wavelengths (e.g., towards the red portion of the spectrum, hence the term “red-shifted.”) This systematic red-shift of extragalactic spectra
was first discovered nearly a hundred years ago, by combining spectra obtained
by V.V. Slipher at Lowell Observatory with distance determinations obtained by
E. Hubble at Mt. Wilson Observatory. 


           Any cosmological theory must explain this observational fact. According
to the Big Bang theory, the observed red-shifts are a direct consequence of
the expansion of the Universe since the Big Bang (13.7 billion years ago).
As space(time) expands, the light-waves stretch with the space they are in,
meaning their wavelengths get longer, or red-shifted.


 Timeline of the universe, showing the formation of particles, then nebula, then more.


     b) There is remnant radiation observed in all directions of space, corresponding
to a temperature of 2.73 Kelvins (above absolute zero), peaking at a wavelength of
~1 millimeter, which is in the “microwave” region of the electromagnetic spectrum.


         Any cosmological theory must explain why we see this radiation uniformly
in all directions in the sky.  According to the Big Bang theory, early in the
Universe’s history, its state was extremely hot and dense–so hot that
protons and electrons were separated from each other in a state
known as a “plasma.” Photons (light) cannot escape such a plasma,
since photons strongly interact with free electrons and protons. This
interaction is called “scattering.”  As the Universe expands, it cools. Once the Universe
had expanded and cooled enough so that protons and electrons
could combine to form atoms, the plasma turned into an electrically
neutral state, and the photons could escape–so instead of a dense, opaque
fog of scattered photons, we have a transparent state of freely propagating photons (light).
The microwave background radiation was discovered (accidentally) by some radio
communications engineers (as a source of unwanted noise in their communications
equipment). They received the Nobel Prize in Physics for their discovery.


    c)  We observe the elemental abundances in the Universe to be
~90% (by number) hydrogen and ~10% (by number) helium.
In terms of mass, this corresponds to ~75% by mass of hydrogen and ~24% by mass
helium. All the other elements we are familiar with here on Earth are trace
elements relative to these, on the scale of stars, galaxies, and galaxy clusters.


      The abundances of hydrogen and helium are predicted by the Big Bang theory
in terms of what is known as “Big Bang nucleosynthesis.”


2. Did all of the elements form at once with the Big Bang? And if not, in what order (if any) did they form in?


      The nucleon formation order in the Big Bang was: protons (protons are nuclei
of hydrogen) and neutrons, then deuterons (the nuclei of deuterium or heavy
water), then helium nuclei (both “light” helium, with  2 protons+1 neutron and “regular” helium, with 2 protons + 2 neutrons), then lithium. All the tritium nuclei (12 yr half-life) and beryllium nuclei (53 day half-life) formed in the Big Bang decayed into deuterons or lithium.
  
          All other elements are formed either within massive stars, post-main-sequence stars, supernovae, or spallation of cosmic particles and interstellar hydrogen nuclei (protons).


3. Would it be theoretically possible to create even more elements?


       Yes, elements past uranium, the so-called “trans-uranium” elements
are all formed in the lab with accelerators. Generally, these very heavy
elements are unstable and decay (their nuclei split apart, or undergo “fission”)
in fractions of a second.


4. What elements are “stardust” and nebulae primarily composed of? 


    Interstellar dust is mainly composed of silicates and hydrocarbons.


     Nebulae are generally gas lit up by a nearby light source, which could be
a massive star or star cluster (e.g., Orion nebula) , a white dwarf (planetary
nebulae), a pulsar (Crab nebula), or very young star  (L1551 in Taurus).
Interstellar gas is primarily composed of hydrogen and helium, with  traces of
other, heavier elements.


A flowchart of star formation; protostars aren’t shown in this chart, but would be between the stellar nebula and a fully-formed star.


6. What are neutron stars?

       A neutron star is an object made entirely of neutrons, that has a radius of ~10 km
and contains more than 1.4 solar masses.  Generally, it is a remnant of a
supernova explosion.


7.  And what are protostars?

       A protostar (of which I am one of the co-discoverers) is an object
which is still in the process of forming, with almost all of its mass residing
in an extended (~2000 Earth-Sun distances, or astronomical units) infalling envelope.
Its energy is derived from gravitational infall, and it fuels powerful bipolar
jets of gas, which act to remove its magnetic field and spin energy.


7. You’re currently studying a protostar, the Wasp-Waist Nebula, right? What do scientists hope to learn from protostars, and for what purposes?


    Fantastic! You saw it! Yes, this nebula is mostly composed of hydrogen.
The protostar forming at the center of the Wasp-Waist Nebula may be the
first such object we have found that ultimately may form into a “failed star”
or “brown dwarf” (an object not massive enough to fuse hydrogen into helium
in its core) instead of into a low-mass star.


        We’re hoping to understand, in detail, both how stars form from the
tenuous interstellar medium and how their planetary systems form.


The Wasp-Waist Nebula, which holds a protostar currently being studied.


8. Do orbiting planets form already orbiting a star? Or do they form, and then drift in space until a sizeable star is encountered?


     Actually, as stars form they form accretion disks, as well. Just like when
water goes down a drain, it generally swirls around before going down the center,
so gas and dust swirl around in a disk around the central protostar before falling in.
Planets eventually form from the disk orbiting the central young (pre-main-sequence,
or, not yet fusing hydrogen to helium) object.


9. Why are the outer planets all gas giants while the inner planets are all rock?


      That has to do with the temperature structure of the accretion disk
around a young, pre-main-sequence object. It’s so hot close-in that only
rocky (silicates, iron) planets can form from planetesimals crashing into each other–it’s too
hot for ices to form. Remember that, by far, most of the material in such
a disk is hydrogen, then helium, with just traces of heavier elements.


   Far enough out in the disk, the temperature cools enough so that both
ices (composed of water, carbon monoxide, ammonia) and rocks (silicates)
can form the central cores of planets. Once an icy/rocky core
surpasses about ten Earth masses, its gravitational pull can become
strong enough to hold onto and sweep up the disk’s gas in and near its orbit.
This is how the gas giants Jupiter and Saturn, and the ice giants, Neptune and
Uranus, formed.


10. Is it difficult to study the formations of stars and planets? What obstacles are in the way of studying these formations?


       Yes, it’s difficult, but it’s rewarding. We are very lucky to live in the present
time, when our technology is allowing us to examine star and planet formation
in unprecedented detail.  The ALMA (Atacama Large Millimeter/submillimeter Array)
will revolutionize our understanding of this field.  This instrument (66 telescopes
working as one) was just inaugurated, on March 13, 2013.  https://science.nrao.edu


11. What kind of technology are scientists using to study these formations?


    Very many kinds. The ALMA array, for instance, uses the fastest, specially
made supercomputer (called a “correlator”) to process the signals from
all of its antennas simultaneously every 10 seconds. The receivers for
detecting radiation from the sky are state-of-the-art and are approaching  (or at) the
quantum limit for how faint a signal they will respond to. Its data processing
software and user interface is brand new and continually being written and upgraded.
This is a truly international collaboration, with scientists from Europe,
North America, Taiwan, and Japan all equal partners in its use and development.


     For near-infrared arrays, to find new brown dwarfs
and young free-floating planets, we’re using the largest such devices in existence.
For near-infrared spectroscopy, we’re using a 400-fiber-optic fed
spectrograph (called FMOS) on the Subaru 8.0-meter telescope on Mauna Kea.
for a recent synopsis of this work).


     We’re looking forward to JWST, the successor to Hubble, which will
work in the near- and mid-infrared. That is where we can study star and planet
formation much better than at optical wavelengths, where these objects
are generally invisible.


  12. How do SETI scientists try to find life in the universe?


  Currently, they are using the ATA (Allen Telescope Array),
looking in a specific frequency range (1-10 GHz) for
narrowband signals that might be transmitted by other


   SETI scientists are also studying geology, geophysics, atmospheric
science, and the conditions under which life may first have arisen on our own planet.
They are studying life in extreme environments on Earth, as in under the Antarctic
ice sheet and on the deep ocean floor where sunlight does not penetrate, and pressures
are high, etc.


13. You’re very involved in different fields of astrophysics; how did you realize your interest in astronomy?

   I remember as a little girl of 4 or 5 years old, looking up at the dark sky, seeing the
stars, and wondering.

The night sky over the Church of Good Shepherd; New Zealand tried to get this patch of sky named a World Heritage Site.
 

Come join the Marin Science Seminar during our Astronomy Month presentations! This Wednesday, March 27, Dr. Mary Barsony will be presenting ‘We are Stardust: Genesis of the Elements’. The Marin Science Seminar takes place from 7:30 to 8:30 p.m., in rm. 207 of Terra Linda High School.


Sandra Ning