What is microlensing? How does it enable astronomers to discover extrasolar planets?

Short Answer

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Microlensing is a phenomenon where the gravitational field of a star magnifies the light of a distant star. It helps astronomers discover extrasolar planets because an observable anomaly in the light curve caused by the planet's gravitational field indicates the presence of the planet. Microlensing facilitates the detection of distant and low-mass extrasolar planets.

Step by step solution

01

Understand Microlensing

Microlensing occurs when the gravitational field of a star acts like a lens, magnifying the light of a distant background star. This is based on Albert Einstein's theory of General Relativity which states that massive objects cause a distortion in space-time, which is experienced as gravity.
02

Identify the Role of Microlensing in Discovering Extrasolar Planets

Microlensing helps in the discovery of extrasolar planets or exoplanets. When a lensing star has a planet orbiting it, the planet's gravitational field can affect the light from the background star, resulting in a detectable anomaly in the light curve. This anomaly in the light curve due to the planet help astronomers discover the planet even when they are far from Earth.
03

Explain the Advantage of Microlensing

Microlensing has a crucial advantage in the field of astronomy. Unlike the traditional planet-hunting methods, microlensing can detect distant planets that other methods would miss. It can also identify low-mass planets that orbit relatively far from their stars.

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Most popular questions from this chapter

Why are terrestrial planets smaller than Jovian planets?

The planet discovered orbiting the star 70 Virginis (" \(70 \mathrm{Vir}\) " in Figure 8-17), 59 light-years from Earth, moves in an orbit with semimajor axis \(0.48 \mathrm{AU}\) and eccentricity \(0.40\). The period of the orbit is \(116.7\) days. Find the mass of 70 Virginis. Compare your answer with the mass of the Sun. (Hint: The planet has far less mass than the star.)

Because of the presence of Jupiter, the Sun moves in a small orbit of radius \(742,000 \mathrm{~km}\) with a period of \(11.86\) years. (a) Calculate the Sun's orbital speed in meters per second. (b) An astronomer on a hypothetical planet orbiting the star Vega, 25 light- years from the Sun, wants to use the astrometric method to search for planets orbiting the Sun. What would be the angular diameter of the Sun's orbit as seen by this alien astronomer? Would the Sun's motion be discernible if the alien astronomer could measure positions to an accuracy of \(0.001\) arcsec? (c) Repeat part (b), but now let the astronomer be located on a hypothetical planet in the Pleiades star cluster, 360 light-years from the Sun. Would the Sun's motion be discernible to this astronomer?

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