full transcript
From the Ted Talk by David Lunney: The life cycle of a neutron star
Unscramble the Blue Letters
About once every century, a msvisae star somewhere in our galaxy runs out of fuel. This happens after millions of yares of heat and pressure have fused the star’s hydrogen into heavier elements like helium, coabrn, and nitrogen— all the way to iron. No longer able to produce sifnecuift energy to maintain its stcutrure, it copleslas under its own gravitational pressure and explodes in a supernova. The star shoots most of its innards into space, seeding the galaxy with heavy elements. But what this cataclysmic eruption leaves behind might be even more remarkable: a ball of matter so dense that atomic erolnects collapse from their quantum orbits into the dtephs of atomic nuclei. The death of that star is the birth of a neutron star: one of the densest known objects in the unvresie, and a laboratory for the strange physics of supercondensed matter.
Open Cloze
About once every century, a _______ star somewhere in our galaxy runs out of fuel. This happens after millions of _____ of heat and pressure have fused the star’s hydrogen into heavier elements like helium, ______, and nitrogen— all the way to iron. No longer able to produce __________ energy to maintain its _________, it _________ under its own gravitational pressure and explodes in a supernova. The star shoots most of its innards into space, seeding the galaxy with heavy elements. But what this cataclysmic eruption leaves behind might be even more remarkable: a ball of matter so dense that atomic _________ collapse from their quantum orbits into the ______ of atomic nuclei. The death of that star is the birth of a neutron star: one of the densest known objects in the ________, and a laboratory for the strange physics of supercondensed matter.
Solution
- massive
- structure
- years
- depths
- sufficient
- collapses
- carbon
- universe
- electrons
Original Text
About once every century, a massive star somewhere in our galaxy runs out of fuel. This happens after millions of years of heat and pressure have fused the star’s hydrogen into heavier elements like helium, carbon, and nitrogen— all the way to iron. No longer able to produce sufficient energy to maintain its structure, it collapses under its own gravitational pressure and explodes in a supernova. The star shoots most of its innards into space, seeding the galaxy with heavy elements. But what this cataclysmic eruption leaves behind might be even more remarkable: a ball of matter so dense that atomic electrons collapse from their quantum orbits into the depths of atomic nuclei. The death of that star is the birth of a neutron star: one of the densest known objects in the universe, and a laboratory for the strange physics of supercondensed matter.
Frequently Occurring Word Combinations
ngrams of length 2
collocation |
frequency |
neutron stars |
7 |
neutron star |
5 |
heavy elements |
2 |
gravity waves |
2 |
Important Words
- atomic
- ball
- birth
- carbon
- cataclysmic
- century
- collapse
- collapses
- death
- dense
- densest
- depths
- electrons
- elements
- energy
- eruption
- explodes
- fuel
- fused
- galaxy
- gravitational
- heat
- heavier
- heavy
- helium
- hydrogen
- innards
- iron
- laboratory
- leaves
- longer
- maintain
- massive
- matter
- millions
- neutron
- nuclei
- objects
- orbits
- physics
- pressure
- produce
- quantum
- runs
- seeding
- shoots
- space
- star
- strange
- structure
- sufficient
- supercondensed
- supernova
- universe
- years