Here is a passage for practicing Reading Skills in IELTS. Solve the questions and find the strategy for solving the passage at the end of the page. If you want to succeed in the next attempt, you must go ahead and join the IELTS reading course. This is the best IELTS preparation course for the aspirants so that they get all the required material
Pointers to keep in mind:
- Time is of the essence, so always make sure you finish solving the exercise in 12mins.
- Do not take external help, this exercise is to help you evaluate your skills.
- Do not look at the answers section till you have finished answering the questions yourself.
- There are 5 parts to the exercise, all are compulsory.
- Spend the first 10 mins finding the answer. Allocate 2 mins to finding the answer to one question.
- After having found all the answers, fill the answer sheet in the last 2 mins.
Understanding the Black Hole
A A black hole is a region in space where the pulling force of gravity is so strong that light is not able to escape. The strong gravity occurs because matter has been pressed into a tiny space. This compression can take place at the end of a star’s life. Some black holes are a result of dying stars. Because no light can escape, black holes are invisible. However, space telescopes with special instruments can help find black holes. They can observe the behaviour of material and stars that are very close to black holes.
B Black holes can come in a range of sizes, but there are three main types of black holes. The black hole’s mass and size determine what kind it is. The smallest ones are known as primordial black holes. Scientists believe this type of black hole is as small as a single atom but with the mass of a large mountain. The most common type of medium-sized black holes is called “stellar.” The mass of a stellar black hole can be up to 20 times greater than the mass of the sun and can fit inside a ball with a diameter of about 10 miles. Dozens of stellar mass black holes may exist within the Milky Way galaxy. The largest black holes are called “supermassive.” These black holes have masses greater than 1 million suns combined and would fit inside a ball with a diameter about the size of the solar system. Scientific evidence suggests that every large galaxy contains a supermassive black hole at its center. The supermassive black hole at the center of the Milky Way galaxy is called Sagittarius A. It has a mass equal to about 4 million suns and would fit inside a ball with a diameter about the size of the sun.
C Primordial black holes are thought to have formed in the early universe, soon after the big bang. Stellar black holes form when the center of a very massive star collapses in upon itself. This collapse also causes a supernova, or an exploding star, that blasts part of the star into space. Scientists think supermassive black holes formed at the same time as the galaxy they are in. The size of the supermassive black hole is related to the size and mass of the galaxy it is in.
D A black hole cannot be seen because of the strong gravity that is pulling all of the light into the black hole’s center. However, scientists can see the effects of its strong gravity on the stars and gases around it. If a star is orbiting a certain point in space, scientists can study the star’s motion to find out if it is orbiting a black hole. When a black hole and a star are orbiting close together, high-energy light is produced. Scientific instruments can see this high-energy light. A black hole’s gravity can sometimes be strong enough to pull off the outer gases of the star and grow a disk around itself called the accretion disk. As gas from the accretion disk spirals into the black hole, the gas heats to very high temperatures and releases X-ray light in all directions. NASA telescopes measure the X-ray light. Astronomers use this information to learn more about the properties of a black hole.
E Black holes do not wander around the universe, randomly swallowing worlds. They follow the laws of gravity just like other objects in space. The orbit of a black hole would have to be very close to the solar system to affect Earth, which is not likely. If a black hole with the same mass as the sun were to replace the sun, Earth would not fall in. The black hole with the same mass as the sun would keep the same gravity as the sun. The planets would still orbit the black hole as they orbit the sun now.
F The sun does not have enough mass to collapse into a black hole. In billions of years, when the sun is at the end of its life, it will become a red giant star. Then, when it has used the last of its fuel, it will throw off its outer layers and turn into a glowing ring of gas called a planetary nebula. Finally, all that will be left of the sun is a cooling white dwarf star.
Reading passage 1 has six paragraphs, A-F.
Match the following information 1-5 to their respective paragraphs.
- The reason why a black hole can’t be seen.
- Formation of black holes
- Why a black hole can’t affect earth
- Types of black holes
- The destiny of sun at the end of its life
Strategies to find information in the passage
Step1: Read the passage.
Read the passage carefully and after reading the passage and the questions, highlight the answers you spotted easily.
Step 2: Spot Keywords
For the answers you did not find, go through the passage again paragraph by paragraph. Underline the keywords you recognize.
Step 3: Before writing the answer
After you think you have found all the answers recheck if your answer clearly addresses the question. Then carefully transfer the answers to the answer sheet.
The answer to the first part of the exercise is D. Answer to the second sub-part lies in the 1st paragraph i.e. A, while the 3rd subpart’s answer can be found in the paragraph E. The heading ‘types of black holes ’ can be found in paragraph B and the answer to the 5th part is F.
You should visit the IELTS Ninja website to get all the details about all the sections of the IELTS exam. Moreover, join the IELTS reading course to know the ways to answer. It is the best IELTS Preparation course for the aspirants.