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A star ignites when its formative gas                                          ‘heavy  hydrogen’  —  has  a  neutron
 cloud collapses, due to its own grav-                                          and  a  proton  in  its  nucleus,  unlike
 itational  pressure  or  some  outside                                         normal hydrogen, which only has a
 force  (such as  the  shockwave  of  a                                         single  proton.  The  fusion of deute-
 supernova blast), to the point where                                           rium is one  of the  very  simplest  of
 the  mass  of the  core  reaches the                                           fusion reactions and requires only a
 temperature  and pressure  needed                                              fraction of the temperature needed
 for hydrogen fusion. But what hap-                                             for hydrogen fusion. Translated into
 pens if such a cloud core just isn’t                                           mass  and gravitational  pressure,
 dense or massive enough to form a                                              this  temperature  requirement  (give
 fully-fledged star? What if the result-                                        or take a couple of tens of thousands
 ing ball  of gas, called a  ‘protostar’,                                       of  kelvin,  depending  on  the  sur-
 lacks the ‘final punch’, so to speak,                                          rounding dust, debris and magnetic
 to begin the process of fusing hydro-                                          fields)  yields  the  ‘thirteen  Jupiter’
 gen?                                                                           threshold. These protostars are hot
 In 1975, the                                                                   and dense enough to fuse deuterium
 For  a  protostar  to  begin  hydrogen                                         with a proton into helium-3. It’s also
 fusion  it  needs  a  core  temperature   astronomer Jill                      the reason why explorers find some
 of  over  one  hundred  million  kelvin.   Tarter came up                      very big gas giants to be rich in he-
 That’s a very high bar which requires                                          lium. The fusion process may have
 immensely  strong  gravitation.  The   with the name                           stopped long ago, but the helium is
 generally accepted lower mass limit   ‘brown dwarf’.                           retained.
 is eight percent of the mass of Sol.
                                                                                Looking for a suitable classification
 Below  this,  hydrogen  fusion  just                                           for  these  substellar  objects,  20th
 isn’t possible as the protostar’s core                                         century  astronomers  considered  a
 temperature  and  pressure  are  too                                           number of terms. ‘Dwarf’ seemed ap-
 low. Astrophysicists have adopted a                                            propriate, as the cosmos had already
 different  scale  for  such  protostars:                                       seen  red  dwarfs  and  white  dwarfs.
 one  based on the  mass  of  Jupiter.                                          They weren’t white, though — rather,
 Protostars  with  between  thirteen                                            they were very, very dim. The terms
 and eighty Jupiter masses become                                               ‘red’ and ‘black’, on the other hand,
 brown dwarfs.                                                                  were  already  occupied;  so  in  1975,
                                                                                the  astronomer  Jill  Tarter  came  up
 Thirteen Jupiter  masses  is  an im-                                           with the name ‘brown dwarf’. In the
 portant  threshold  for  astronomers,                                          absence of better alternatives, this
 because  above  that  point,  another                                          name  has  stuck, and it  is  certainly
 interesting  thermonuclear  process                                            in-keeping with astronomers’ knack
 begins:  the  fusing  of  deuterium.                                           for dramatic terms.
 Deuterium —  sometimes known as
















 58  ISSUE 25 | q4 3305                                                                        ISSUE 25 | q4 3305  59
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