Astronomy Habitable Zone

Astronomy Habitable Zone

Astronomy Habitable Zone , The presence of liquid water is considered to be a prerequisite for life as we know it, which makes looking for water a practical way to begin our search for life beyond Earth. For water to exist on the surface of a planet, the planet must have the right temperature on its surface. The main driving force behind the surface temperature of any planet is the light it receives from its parent star. Around every star there is a region where the planet will receive just the right amount of light to give it temperatures that are conducive to liquid water – this region is call the star’s Habitable Zone. The orbit of the Earth currently falls within the Habitable Zone of our Sun.

2 The Habitability of the Earth

To begin, load up the Habitable Zone simulator written by the University of Nebraska by entering the following URL in the address bar of your web browsers:

http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html

The flash simulator will show you a visual diagram of the solar system in the top panel, a set of simulation settings in the middle panel, and a timeline of the habitability of the Earth in the bottom panel. To run the simulation, click the run in the bottom panel. This button immediately becomes a pause button which will allow you to pause the simulation at any time. To restart the simulation, press the restart button at the very top of the simulation.

The blue region marked on the diagram is the Habitable Zone around our Sun. Notice how there is both an inner edge and an outer edge – the planets interior to the habitable zone are too hot to support liquid water, while the planets exterior to it are too cold.

1) The simulation is currently set to zero-age – this is the Solar System as it was when it first formed, 5 billion years ago. Which planets were in the Habitable Zone at this time?

1

http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html

2) Press the start button and watch the Habitable Zone change with time. Pause the simulation when it reaches an age of 5 billion years (you can keep track of the time by looking at the timeline marker in the bottom panel). This is the Solar System as it is today – which planets are in the Habitable Zone now?

3) Allow the simulation to run until the Earth is no longer in the Habitable Zone. At what age does this happen? How long from now until this happens? You can use the timeline bar in the bottom panel to determine your answers. .

4) After the Earth is no longer within the Habitable Zone, what do you think the condi- tions on Earth will be like?

5) Resume the simulation and let it run until the end. Which planets other than the Earth fell within the Habitable Zone at any point during the Sun’s life?

6) If you had to choose planets of our Solar System for future colonization based on their future habitability, which would you choose, and why?

3 The Habitability Different Kinds of Stars

Now that you’ve simulated the Habitable Zone around our Sun, we’ll run the same simulation for other stars. Astronomers classify stars with letters, O, B, A, F, G, K, and M. The O stars are the hottest and brightest, while the M stars are the dimmest and coolest. Every kind of star has a Habitable Zone, but the brighter the star the farther out the Habitable Zone. Imagine putting and extra log on a campfire – the campers all have back off a few feet to maintain the same comfortable temperature.

But in order for complex life to have a chance to develop, a planet must remain habitable for an extended period of time. How long? We only have Earth to use as an example, so we really don’t know. For the purpose of this exercise, we’ll assume that Earth is “typical” and that planets around other stars mostly follow the timeline of events on Earth shown below:

2 Billions of Years Ago Development Toward Complex Life 4.5 Earth forms 4.3-4.4 Earth cools, oceans form 3.8 first bacterial fossils 2.4 rise of oxygen in atmosphere 2.0 first complex cells 0.55 first complex animals (fossils in Clapp)

The next table shows several different kinds of stars. Notice how they each have a different mass – the mass of a star determines what kind of a star it is. Reset the Habitable Zone simulator with the reset button at top, and then adjust the star mass with the initial star mass slider bar in the middle panel. Notice how the Habitable Zone immediately changes size. Notice also that you can adjust the orbit of “Earth” by adjusting the initial planet distance slider bar in the middle panel. The units of distance from the star are AU – astronomical units, the distance of the Earth from the Sun. The Earth is one AU from the Sun.

For each of the star types in the table below, find the planet orbit that remains habitable the longest. To do this you’ll need to run the simulation many times for each star type, each time adjusting the initial planet distance until you find a distance that keeps the planet habitable the longest. Record in the table 1) the size of this orbit, in AU, 2) how long this orbit remains habitable, 3) the most advanced type of life that can develop during this time frame, assuming the Earth’s timeline for life is typical.

Type Star Mass Longest Habitable Orbit Habitable Lifetime Most Advanced Life [Solar Masses] [Astronomical Units] [Billions of Years]

O 15. B 5.0 A 2.0 F 1.3 G (Sun) 1.0 K 0.7 M 0.4

4 Tidal Locking

Unfortunately, for low-mass M type stars the habitable zone is quite close to the star – so close that planets in this zone are likely to be tidally locked. This means that the same side of the planet will always face the star, just as the same side of the Earth’s moon always faces the Earth. The simulator indicates that a planet is tidally locked when it is split between one brown and the other side being light gray. In this section we’ll experiment with planets around M type stars. Adjust the stars “initial stellar mass” to 0.3 (30% of the Sun’s mass), and adjust the “initial planet distance” until the planet is in the star’s Habitable Zone. The planet should switch to the tidally locked icon, even if the planet is in the Habitable Zone.

1) What impact do you think tidal locking would have on the prospect of life on this planet?

2) Try adjusting the star’s mass. What is the lowest mass star that would allow a non- tidally locked planet in the Habitable Zone at the beginning of the star’s life?

3) What is the lowest mass star that would allow a non-tidally locked planet in the Hab- itable Zone at any point during the star’s life?

5 Tying it All Together

1) Given what you’ve learned so far, what type of star is the best place to look for life?

2) The Sun is a G-type star. What do you think the development of life on planets orbiting hotter types of stars would be like? What about cooler types of stars? Do you think that life in such conditions is even possible? Justify your answer.

3) If you were the director of a NASA program to search for life beyond Earth, toward which type of star would you direct your attention? Why? Justify your answer using the evidence above, and also any other lines of reasoning you like. Help Me Write My Essay

HelpHub
Calculate your paper price
Pages (550 words)
Approximate price: -

Why Choose HelpHub

HelpHub

Quality Researched Papers

We always make sure that writers follow all your instructions precisely. You can choose your academic level: high school, college/university or professional, and we will assign a writer who has a respective degree.

HelpHub

Qualified Writers

We have hired a team of professional writers experienced in academic and business writing. Most of them are native speakers and PhD holders able to take care of any assignment you need help with.

StudyAcer

Unlimited Revisions

If you think we missed something, send your order for a free revision. You have 10 days to submit the order for review after you have received the final document. You can do this yourself after logging into your personal account.

StudyAcer

On Time Delivery

All papers are always delivered on time. In case we need more time to master your paper, we may contact you regarding the deadline extension. We will always strive to deliver on time.

StudyAcer

Original & Confidential

We use several writing tools checks to ensure that all documents you receive are free from plagiarism. Our editors carefully review all quotations in the text.

StudyAcer

24/7 Customer Support

Our support agents are available 24 hours a day 7 days a week and committed to providing you with the best customer experience. Get in touch whenever you need any assistance.

Try it now!

Calculate the price of your order

Total price:
$0.00

How it works?

Follow these simple steps to get your paper done

Help Hub

Place your order

Fill in the order form and provide all details of your assignment.

Help Hub

Proceed with the payment

Choose the payment system that suits you most.

Help Hub

Receive the final file

Once your paper is ready, we will email it to you.

HelpHub Writing Services

No need to work on essay at night. Sleep tight, we will cover your back. We offer all kinds of essay writing services.

HelpHub HelpHub

Essays

Essay Writing Service

No matter what kind of academic paper you need and how urgent you need it, you are welcome to choose your academic level and the type of your paper at an affordable price. We take care of all your paper needs and give a 24/7 customer care support system.

HelpHub HelpHub

Admissions

Admission Essays

An admission essay is an essay or other written statement by a candidate, often a potential student enrolling in a college, university, or graduate school. You can be rest assurred that through our service we will write the best admission essay for you.

HelpHub HelpHub

Editing

Editing Support

Our academic writers and editors make the necessary changes to your paper so that it is polished. We also format your document by correctly quoting the sources and creating reference lists in the formats APA, Harvard, MLA, Chicago / Turabian.

HelpHub HelpHub

Revision

Revision Support

If you think your paper could be improved, you can request a review. In this case, your paper will be checked by the writer or assigned to an editor. You can use this option as many times as you see fit. This is free because we want you to be completely satisfied.