the hunt for exoplanets

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Essay on Exoplanet

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Page 1: The Hunt for Exoplanets

Essay on Exoplanet

Page 2: The Hunt for Exoplanets

Table of content

Contents

Introduction ................................................................................................................................... 2

Exoplanets ................................................................................................................................... 2

First Exoplanet: 51 Pegasi b........................................................................................................ 2

Total Exoplanets discovered ....................................................................................................... 2

Aim of the Report........................................................................................................................ 3

The methods of searching Exoplanets .......................................................................................... 4

The stars we are looking for ........................................................................................................ 4

‘Super Earths’ and ‘Hot Jupiters’ ................................................................................................ 4

The concept of a “Habitable Zone” ............................................................................................. 4

The techniques of detecting Exoplanets ...................................................................................... 4

The radial velocity method ...................................................................................................... 5

The astrometry method ............................................................................................................ 5

The transit method ................................................................................................................... 5

Spectroscopic Analyses to determine a ‘Fingerprint’ of life ....................................................... 6

Recent Discoveries.......................................................................................................................... 7

Key Discoveries .......................................................................................................................... 7

51 Pegasi b ............................................................................................................................... 7

Proxima Centuari b .................................................................................................................. 7

WASP-33b ............................................................................................................................... 7

Proxima Centuari b and WASP-33b ........................................................................................... 7

Conclusions ..................................................................................................................................... 9

References ..................................................................................................................................... 10

Page 3: The Hunt for Exoplanets

Introduction

Humanity is evolving ever since the inception of the journey on earth. Learning new things and

discovering the unseen is in the roots of the evolution process. In the modern era, science doesn’t

believe that Sky is the limit rather it has expanded their span of research to the infinite space. Space

research has uncovered some mesmerising phenomenon which is lifting the human evolution to

the next level (Barge & Others, 2008).

Exoplanets

The curiosity to find earth-like planet can be dated to long time ago. But because of the incapability

of the available technologies, it was a dream to detect planets beyond our solar system. After the

time stated, the space research have taken a new leap and opened a new era of information. The

concept of Exoplanet born. It can also be referred to as Extra Solar Planet. Any planet which is not

within our solar system is Exoplanet. But an absolute definition is quite complex and problematic.

So some of the important characteristics of an Exoplanet is it has to be earth-like environment, it

can be giant or terrestrial type (Astronomy, 2017).

First Exoplanet: 51 Pegasi b

The first ever Exoplanet was discovered in October 1995 by Didier Queloz and Michel Mayor of

Geneva University. The planet was orbiting a star named 51 Pegasi and the planet was named after

it in a poetic way, 51 Pegasi b. The planet is 300 trillion miles away from our solar system. Actually

it is the inception point of Exoplanet chapter in space research. It is assumed that the surface

temperature of the planet is 1,000C and it is orbiting the sun in just 4 days. Because of its mass

and temperature, the Exoplanet is a “Hot Jupiter” kind of Exoplanet (Bbc.co.uk, 2017).

Total Exoplanets discovered

Since the discovery of 51 Pegasi b, thousands of new planets in different solar system has been

discovered. Till the date, a total of around 3,440 Exoplanets has been discovered. There are

different medium as well method through which the Exoplanets are confirmed. NASA’s Kepler is

one of the crucial in this case (Astronomy, 2017). Most of the planets are confirmed using transit

method. The table is given below –

Page 4: The Hunt for Exoplanets

Aim of the Report

The report is dedicated to provide a short description on the methods of discovering Exoplanets

and some of the recent and key discoveries in the Exoplanets using those methods

Page 5: The Hunt for Exoplanets

The methods of searching Exoplanets

Search for a habitable planet is quite a complex process and still we are far behind to be perfect in

searching for a suitable planet like earth. Today’s modern technologies doesn’t allow us to

perfectly identify an Exoplanet but there are some methods available for this purpose

The stars we are looking for

The priority at the time of looking for an Exoplanet is to find a habitable planet. The Exoplanetary

system should have a CHZ which is Circumstellar Habitable Zone. The zone must inhibit into a

stable star system. The probability of having CHZ will increase in such situation. The star system

should also have the presence of water (@JosephStromberg, 2017).

‘Super Earths’ and ‘Hot Jupiters’

There are a number of planets that can be considered at the time of the exploration of the space.

Hot Jupiters and Super Earths are most desired one. Hot Jupiters are referred to the exoplanets

which is similar to our solar system’s planet Jupiter in terms of mass but generally has short orbital

radii and a semi-major axes somewhere near .015 to .5 which can be converted to an astronomica l

unit of .2×106 to 74.8×106 km. The word hot is added to the phenomenon because of the high

surface temperature of the planet (worldcrunch, 2017)

Super Earths refers to exoplanets which are much like earth with a higher mass. The term doesn’t

include any reference to the habitability of the planet, the surface condition or the environment. It

is total tagged with the mass of the earth (Exoplanetarchive.ipac.caltech.edu., 2017).

The concept of a “Habitable Zone”

The critical characteristics for “Habitable Zone” is the distance with the star so the liquid doesn’t

vaporize or freeze. Although the inception definitions were only concentrated on the thermal

equilibrium, the latest development also include the required gravitational pull caused by large

planets which allows it to generate essential energy for blooming life.

The techniques of detecting Exoplanets

Page 6: The Hunt for Exoplanets

As there are still some major limitations in the space research technologies, the advancements are

also praiseworthy. There are mainly three major techniques to detect Exoplanets. The focus of all

the techniques intertwined with its star. The major techniques are explained below –

The radial velocity method

Redial Velocity is one of the most useful methods in the exoplanetary research. This method focus

on the lights from the star and let it pass through a prism to split into spectrum. The spectrum is

then magnified which creates straight black lines on the usual colours. The spectral lines is parallel

to the wavelength of light which is originated from the star and absorbed the chemicals of the

planet. Every chemical has its own wavelength so is different from one another and can tell the

characteristics of the source. Studying these spectre lines is all we need to know about the planet

(European Space Agency., 2017).

The astrometry method

Other than spectre analysis, the exoplanet can also be detected by measuring the exact position of

a star. As a result the wobbling can be directly detected. Hubble space telescope is used for this

purpose (Wright & Others, 2011). But it is hard to accord these detections with the modern

methods. So, it is not possible to confirm the detections. Gaia is one the most perfect astrometric

satellite in the current data. The estimated data to processed using the satellite is around thousand

million stars. Once again, however, the wobbling motion caused by an Earth-sized planet will be

too small to be detectable, even by Gaia (AMNH., 2017).

The transit method

Another very promising method for detecting exoplanets is the transit method. In this method, the

major focus is on the fluctuation in the level of light due to the planet transiting through the star.

When a planet pass through a star, there is a subtle deviation in the emission of light of that sun.

For example, when Jupitar pass through, there is almost a 1 percent loss of light. This method has

gave us a total of 10 planets and is more promising method than others.

Other than these three major techniques, direct detection and imaging, Doppler isolation,

polarimetry, nulling interferometry, seeing more with space telescopes are also some of the other

popular techniques for detecting Exoplanets (Snellen & Others, 2010).

Page 7: The Hunt for Exoplanets

Spectroscopic Analyses to determine a ‘Fingerprint’ of life

According to Kreidberg & Others (2014) the fingerprint of life out in the space is detected using

the spectroscopic analysis. In this particular method, the light of the exoplanet is used. When we

try to determine whether the planet have an atmosphere or not, we analyse light that pass from the

atmosphere. When the light of a star pass through the atmosphere of a planet, substance of the

atmosphere absorb certain wavelength is a symbolic way. When we analyse the light of the planet,

it bears the signature of different chemical. If the spectroscopic analysis found that there is ample

amount of oxygen, water, CO2 and methane in the atmosphere, their might be a possibility of life

on that planet (Earth 2.0., 2017).

Page 8: The Hunt for Exoplanets

Recent Discoveries

In the infinite space, there are billions of planets and we have already discovered more than 2,000

planets. So, it is a little complex to narrow down these into a few planets. After considering a

number of factors, the key discoveries in the field are –

Key Discoveries

51 Pegasi b

The exoplanet journey was started from this point so 51 Pegasi b is one of the key discoveries. The

planet is categorised under the hot Jupiter and the distance with sun is roughly similar to Mercury

to sun. Because of the phenomenon, one side of the planet is always facing the sun (Wasp-

planets.net., 2017).

Proxima Centuari b

It has been officially confirmed that Proxima Century b, a red dwarf star, is only 4.25 light years

away from earth. The planet is confirmed using the Redial Velocity method in August, 2016. It is

slightly closer to the famous binary pair Alpha Centauri A and B. It has been estimated that the

mass is roughly 1.3 times that of earth (Gizmodo.com, 2017).

WASP-33b

This planet was discovered in 2011 and has a sort of "sunscreen" layer — a stratosphere — that

absorbs some of the visible and ultraviolet light from its parent star. Not only does this planet orbit

its star "backward," but it also triggers vibrations in the star, seen by the MOST satellite (WrightDr,

2013).

Proxima Centuari b and WASP-33b

It has been officially confirmed that Proxima Century b, a red dwarf star, is only 4.25 light years

away from earth. The planet is confirmed using the Redial Velocity method in August, 2016. It is

slightly closer to the famous binary pair Alpha Centauri A and B. It has been estimated that the

mass is roughly 1.3 times that of earth. It is within the habitable zone for exoplanet. The

environment is also habitable and water is in the liquid form (Mason, 2008). It’s not yet clear

whether this new exoplanet has an atmosphere. Because Proxima Centauri is a fairly active star,

Page 9: The Hunt for Exoplanets

Proxima b suffers x-ray fluxes approximately 400 times greater than what we experience here on

Earth, and this could cause any atmosphere to blow away.WASP-33 is a planet which is an

important contributors in the hot Jupiter category. The planet is very close to its star and the

temperature is quite off the chart. The planet is confirmed in 2010 using the transit method (Deleuil

& Others, 2008).

Page 10: The Hunt for Exoplanets

Conclusions

The essay is about the detection methods for the exoplanets and some recent important discoveries,

some of the important facts included in the essay. Moreover, there are some limitations in the

technology but the advancement in the sector quite praiseworthy. If science will excel in this rate,

we can hope that in the near future, we might be vising any nearby planet for the habitation

purpose. A lot of things has turned into reality from science fiction. Space research is that why an

exciting thing.

Page 11: The Hunt for Exoplanets

References

@JosephStromberg, F. (2017). How Do Astronomers Actually Find Exoplanets?. [online] Smithsonian.

Available at: http://www.smithsonianmag.com/science-nature/how-do-astronomers-actually-find-

exoplanets-180950105/ [Accessed 30 Jan. 2017].

Earth 2.0. (2017). The search for Earth 2.0. [online] Available at:

https://www.1843magazine.com/content/features/george-pendle/exoplanets [Accessed 30 Jan. 2017].

AMNH. (2017). The Hunt for Extrasolar Planets. [online] Available at:

http://www.amnh.org/explore/science-bulletins/astro/documentaries/beyond-our-solar-system-searching-

for-extrasolar-planets/the-hunt-for-extrasolar-planets/ [Accessed 30 Jan. 2017].

World Crunch, (2017). [online] Available at: http://www.worldcrunch.com/chemical-fingerprints-what-

planets-reveal-about-alien-life-forms/tech-science/chemical-fingerprints-what-the-planets-reveal-about-

alien-life-forms/c4s5498/#.UK1EKuOe98w [Accessed 30 Jan. 2017].

Astronomy, S. (2017). Exoplanets: Worlds Beyond Our Solar System. [online] Space.com. Available at:

http://www.space.com/17738-exoplanets.html [Accessed 30 Jan. 2017].

Astronomy, S. (2017). The Hunt for Exoplanets Heats Up. [online] Space.com. Available at:

http://www.space.com/26554-the-hunt-for-exoplanets-heats-up.html [Accessed 30 Jan. 2017].

Barge, P., Baglin, A., Auvergne, M., Rauer, H., Léger, A., Schneider, J., Pont, F., Aigrain, S., Almenara,

J.M., Alonso, R. and Barbieri, M., 2008. Transiting exoplanets from the CoRoT space mission-I. CoRoT-

Exo-1b: a low-density short-period planet around a G0V star. Astronomy & Astrophysics, 482(3), pp.L17-

L20.

Bbc.co.uk. (2017). BBC Universe - 51 Pegasi: The first exoplanet around a Sun-like star. [online]

Available at: http://www.bbc.co.uk/science/space/universe/key_places/51_pegasi [Accessed 30 Jan.

2017].

Deleuil, M., Deeg, H.J., Alonso, R., Bouchy, F., Rouan, D., Auvergne, M., Baglin, A., Aigrain, S.,

Almenara, J.M., Barbieri, M. and Barge, P., 2008. Transiting exoplanets from the CoRoT space mission-

VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert. Astronomy &

Astrophysics,491(3), pp.889-897.

European Space Agency. (2017). How to find an extrasolar planet. [online] Available at:

http://www.esa.int/Our_Activities/Space_Science/How_to_find_an_extrasolar_planet [Accessed 30 Jan.

2017].

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Exoplanetarchive.ipac.caltech.edu. (2017). Exoplanet Archive Planet Counts. [online] Available at:

http://exoplanetarchive.ipac.caltech.edu/docs/counts_detail.html [Accessed 30 Jan. 2017].

Gizmodo.com. (2017). Cite a Website - Cite This For Me. [online] Available at: http://gizmodo.com/new-

earth-like-exoplanet-could-be-discovery-of-the-cent-1785614793 [Accessed 30 Jan. 2017].

Kreidberg, L., Bean, J.L., Désert, J.M., Benneke, B., Deming, D., Stevenson, K.B., Seager, S., Berta-

Thompson, Z., Seifahrt, A. and Homeier, D., 2014. Clouds in the atmosphere of the super-Earth exoplanet

GJ [thinsp] 1214b.Nature, 505(7481), pp.69-72.

Mason, J. ed., 2008. Exoplanets: detection, formation, properties, habitability. Springer Science

& Business Media.

Snellen, I.A., De Kok, R.J., De Mooij, E.J. and Albrecht, S., 2010. The orbital motion, absolute mass and

high-altitude winds of exoplanet HD [thinsp] 209458b. Nature, 465(7301), pp.1049-1051.

Wasp-planets.net. (2017). WASP-33b | WASP Planets. [online] Available at: https://wasp-

planets.net/tag/wasp-33b/ [Accessed 30 Jan. 2017].

Wright, J.T., Fakhouri, O., Marcy, G.W., Han, E., Feng, Y., Johnson, J.A., Howard, A.W., Fischer, D.A.,

Valenti, J.A., Anderson, J. and Piskunov, N., 2011. The exoplanet orbit database. Publications of the

Astronomical Society of the Pacific, 123(902), p.412.

WrightDr, J.T., 2013. Exoplanet detection methods. In Planets, Stars and Stellar Systems (pp. 489-540).

Springer Netherlands.