the layered earth: a1 atmospheric composition 3lzzvu 7shu plan/trappist-1 lesson plan.pdfruv^slknl...

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Guiding Question >OH[ HYL L_VWSHUL[Z HUK OV^ PZ [OL ;9(770:; KPZJV]LY` ZPNUPMPJHU[& Key Concepts (U L_VWSHUL[ PZ H WSHUL[ [OH[ VYIP[Z H Z[HY V\[ZPKL VM V\Y V^U ZVSHY Z`Z[LT ,_VWSHUL[Z HYL JVTTVU HYV\UK V[OLY Z[HYZ HUK OH]L ILLU KPZJV]LYLK I` H ]HYPL[` VM TL[OVKZ ;OL OHIP[HISL aVUL PZ H YLNPVU PU ZWHJL HYV\UK H Z[HY [OH[ JV\SK JVUJLP]HIS` Z\WWVY[ SPML ,HY[O:PaLK WSHUL[Z JHU IL MV\UK HYV\UK YLK K^HYM Z[HYZ Introducing the Lesson <U[PS YLJLU[S` V\Y ZVSHY Z`Z[LT ^HZ [OL VUS` WSHUL[HY` Z`Z[LT O\THUZ RUL^ 0[ ^HZ L]LU [OV\NO[ I` ZVTL [OH[ V\Y ZVSHY Z`Z[LT ^HZ \UPX\L PU [OL \UP]LYZL ;OPZ JOHUNLK PU [OL LHYS` Z ^OLU HZ[YVUVTLYZ ILNHU [V KPZJV]LY [OL MPYZ[ L_VWSHUL[Z ^VYSKZ VYIP[PUN V[OLY Z[HYZ :PUJL [OL MPYZ[ KPZJV]LY` HZ[YVUVTLYZ OH]L MV\UK [OV\ZHUKZ VM L_VWSHUL[Z (Z[YVUVTLYZ UV^ ILSPL]L [OH[ WSHUL[HY` Z`Z[LTZ HYL WSLU[PM\S [OYV\NOV\[ [OL \UP]LYZL :JPLUJL MPJ[PVU OHZ ILJVTL ZJPLUJL MHJ[ /\THUP[` PZ UL^ [V O\U[PUN WSHUL[Z V\[ZPKL V\Y ZVSHY Z`Z[LT HUK HZ[YVUVTLYZ OH]L VUS` YLJLU[S` ILLU HISL [V KL[LJ[ [OLZL WSHUL[Z ;OL WYVISLT PZ [OH[ H WSHUL[ PZ T\JO MHPU[LY [OHU P[Z WHYLU[ Z[HY· SLZZ [OHU H IPSSPVU[O HZ IYPNO[ ,]LU [OL SHYNLZ[ HUK IYPNO[LZ[ VM [OLZL L_VWSHUL[Z NL[Z SVZ[ PU [OL NSHYL VM P[Z Z[HY 3\JRPS` [OLYL HYL PUKPYLJ[ ^H`Z VM KL[LJ[PUN L_VWSHUL[Z I` TLHZ\YPUN [OL LMMLJ[Z H WSHUL[ OHZ VU P[Z Z[HY 6UL PZ [V KL[LJ[ [OL NYH]P[H[PVUHS [\N VM H WSHUL[ HZ P[ VYIP[Z P[Z WHYLU[ Z[HY ^OPJO THRLZ [OL Z[HY Z^H` IHJR HUK MVY[O (UV[OLY TL[OVK PZ [V KL[LJ[ [OL KPTTPUN [OH[ VJJ\YZ ^OLU H WSHUL[ WHZZLZ IL[^LLU H Z[HY HUK HU VIZLY]LY IHJR VU ,HY[O Time Required Approximately 60 minutes Voca bula ry Astronomical Unit Exobiologist Exoplanet Habitable Zone Light-year Red Dwarf SkyGuide Lesson Teachable Moments -> Exploring the TRAPPIST-1 Planetary System 3LZZVU 7SHU ,_WSVYPUN [OL ;9(770:; 7SHUL[HY` :`Z[LT The Layered Earth: A1 Atmospheric Composition :[HUKHYKZ *VUULJ[PVU 5.:: +PZJPWSPUHY` *VYL 0KLH! ,HY[OZ 7SHJL PU [OL <UP]LYZL HUK *YVZZJ\[[PUN *VUJLW[Z·7H[[LYUZ :JHSL 7VY[PVU HUK 8\HU[P[`" HUK :`Z[LTZ HUK :`Z[LT 4VKLSZ Grades 5 – 12 :WHJL :`Z[LTZ Grades 9 – 12 :WHJL :`Z[LTZ 5:,: General (IPSP[PLZ ULJLZZHY` [V KV ZJPLU[PMPJ PUX\PY` <UKLYZ[HUKPUN HIV\[ ZJPLUJL HUK [LJOUVSVN` :JPLUJL HZ H O\THU LUKLH]VY 4V[PVUZ HUK MVYJLZ Grades 6 – 8 ;YHUZMLY VM LULYN` ,HY[O PU [OL ZVSHY Z`Z[LT Grades 9 – 12 6YPNPU HUK L]VS\[PVU VM [OL ,HY[O Z`Z[LT www.StarryNight.com

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Page 1: The Layered Earth: A1 Atmospheric Composition 3LZZVU 7SHU Plan/TRAPPIST-1 Lesson Plan.pdfruv^slknl huk i\psk j\ypvzp[` hiv\[ z[hyz l_vwshul[z huk [ol wv[lu[phs vm hsplu spml vu v[oly

Guiding Question>OH[�HYL�L_VWSHUL[Z�HUK�OV^�PZ�[OL�;9(770:;���KPZJV]LY`�ZPNUPMPJHU[&

Key Concepts• (U�L_VWSHUL[�PZ�H�WSHUL[�[OH[�VYIP[Z�H�Z[HYV\[ZPKL�VM�V\Y�V^U�ZVSHY�Z`Z[LT�

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Introducing the Lesson<U[PS�YLJLU[S`��V\Y�ZVSHY�Z`Z[LT�^HZ�[OL�VUS`�WSHUL[HY`�Z`Z[LT�O\THUZ�RUL^��0[�^HZ�L]LU�[OV\NO[�I`�ZVTL�[OH[�V\Y�ZVSHY�Z`Z[LT�^HZ�\UPX\L�PU�[OL�\UP]LYZL��;OPZ�JOHUNLK�PU�[OL�LHYS`�� �Z��^OLU�HZ[YVUVTLYZ�ILNHU�[V�KPZJV]LY�[OL�MPYZ[�L_VWSHUL[Z��^VYSKZ�VYIP[PUN�V[OLY�Z[HYZ�:PUJL�[OL�MPYZ[�KPZJV]LY`��HZ[YVUVTLYZ�OH]L�MV\UK�[OV\ZHUKZ�VM�L_VWSHUL[Z��(Z[YVUVTLYZ�UV^�ILSPL]L�[OH[�WSHUL[HY`�Z`Z[LTZ�HYL�WSLU[PM\S�[OYV\NOV\[�[OL�\UP]LYZL��:JPLUJL�MPJ[PVU�OHZ�ILJVTL�ZJPLUJL�MHJ[�

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Tim e R e quire dApproximately60 minutes

V o c a b u la r yAstronomical UnitExobiologistExoplanetHabitable ZoneLight-yearRed Dwarf

SkyGuide Lesson

Teachable Moments -> Exploring the TRAPPIST-1 Planetary System

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The Layered Earth: A1 Atmospheric Composition

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www.StarryNight.com

Page 2: The Layered Earth: A1 Atmospheric Composition 3LZZVU 7SHU Plan/TRAPPIST-1 Lesson Plan.pdfruv^slknl huk i\psk j\ypvzp[` hiv\[ z[hyz l_vwshul[z huk [ol wv[lu[phs vm hsplu spml vu v[oly

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The TRAPPIST-1 system is a significant discovery for a number of reasons:

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www.StarryNight.com

Page 3: The Layered Earth: A1 Atmospheric Composition 3LZZVU 7SHU Plan/TRAPPIST-1 Lesson Plan.pdfruv^slknl huk i\psk j\ypvzp[` hiv\[ z[hyz l_vwshul[z huk [ol wv[lu[phs vm hsplu spml vu v[oly

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G. How do you think astronomers are able to detect exoplanets around other stars?

Answers from students will vary.

H. If a planet moves in front of its star (a transit), what do you think will happen to the amount of light reaching you?

The amount of light reaching you would diminish for the duration of the transit. The effect is similar to moving a coin in front of a flashlight.

www.StarryNight.com

Page 4: The Layered Earth: A1 Atmospheric Composition 3LZZVU 7SHU Plan/TRAPPIST-1 Lesson Plan.pdfruv^slknl huk i\psk j\ypvzp[` hiv\[ z[hyz l_vwshul[z huk [ol wv[lu[phs vm hsplu spml vu v[oly

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I. Many of the exoplanets that astronomers have discovered are very large and very close to their parent star. Why do you think that is? Why is it harder to find smaller planets?

Transit Photometry - measuring the dimming of a star’s light when its planets pass between us and the star; and Radial Velocity and Stellar Astrometry - two methods that detect the subtle motions of stars caused by orbiting planets tugging on them gravitationally; are some of the most effective methods to detect exoplanets.

It is easier to detect larger planets passing in front of a star and detect the gravitational pull of larger planets on their host star. It is also easier to detect planets if they are orbiting closer to their parent star, as these planets block more light, complete their orbits faster, reflect more light, and can have a greater measurable gravitational effect on their parent star.

J. What makes Earth special compared to other known planets?

Earth is the only known planet in the universe to harbor life.

K. Do you think some exoplanets could support alien life or be habitable by humans? What kinds of criteria should we consider when looking for an exoplanet that might have life?

Our galaxy, the Milky Way, contains up to 400 billion stars. Exoplanets outnumber stars in our galaxy. To date we have also detected many Earth-sized planets at the right distance from their stars to maintain liquid water on their surface. The odds are that a great number of exoplanets in our galaxy alone will be capable of supporting life and be habitable by humans. Odds are also that alien life might be present on some of these worlds.

New tools are being developed that will allow astronomers to look for the telltale signs of life on exoplanets. It will soon be possible to directly detect an analyze the atmosphere of nearby exoplanets. Scientists will be looking for the presence of atmospheric oxygen - a marker that could indicate biological activity.

L. Do you think we’ll keep finding more exoplanets?

Yes. Scientists are developing new tools and techniques to detect exoplanets. New space observatories are also being launched in the next few years that will detect even more Earth-sized exoplanets. Hunting for exoplanets is still in its infancy.

M. All exoplanets discovered so far can be found within our own galaxy, the Milky Way. Do you think other galaxies might also have planets?

Yes. Other galaxies are formed much the same way as our own galaxy, the Milky Way. It is safe to conclude that planets also form around stars in other galaxies.

Extension ActivitiesActivity One: Have your students draw their own exoplanet star system. Have them include details such as the distance to the planets, planet sizes (gas giants, rocky worlds etc), star type (bluer stars are hotter, while redder stars are cooler), planet age, and which ones might be able to support life.

Activity Two: Have students draw and/or write about what it might be like to live on the surface of a TRAPPIST-1 exoplanet.

www.StarryNight.com

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Vocabulary Link

Astronomical Unit: The average distance from the Earth to the sun, or 149,597,870 kilometers (92,955,807 miles). Abbreviated AU.

Exobiologist: Study the branch of biology that deals with the search for extraterrestrial life and the effects of extraterrestrial surroundings on living organisms. Also called astrobiology.

Exoplanet: a planet that orbits a star outside our solar system.

Habitable Zone: The region in space around a star that might potentially support life; surface temperatures of planets in the habitable zone allow for the existence of liquid water.

Light-Year: The distance light travels in one year. One light-year is approximately 9,460,536,000,000 kilometers (5,878,505,000,000 miles).

Red Dwarf: A small and relatively cool star on the main sequence.

Evidence of Learning

Upon completion of this lesson, you should have evidence that students can:

• Explain what an exoplanet is.• Understand some of the methods to detect planets outside our solar system.• Recognize the vast distance between the stars.• Understand the importance of exoplanet research.

Additional Resources

SkyGuide->Teachable Moments->Exoplanets: Worlds Outside Our Solar System

NASA Exoplanet Archive - http://exoplanetarchive.ipac.caltech.edu

www.StarryNight.com