Reach for the Stars Presented by Linder Winter National Event Supervisor Member: E-S Rules...
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Transcript of Reach for the Stars Presented by Linder Winter National Event Supervisor Member: E-S Rules...
The Chandra X-ray CenterSponsors my participation.
Please record your name, e-mail address, and physical address on the sign-in sheet.
The Chandra X-ray Center uses this information to determine which workshops it will continue to support and may contact you to ask whether you are using the Chandra Educational activities.
It is NASA’s policy to not reveal your personal information to others.
Presentation Outline
Resources
1. Clinic website
2. Stellar Journey Game
3. Stellar Cycle Cards
4. Other Worlds Educational Enterprises handout Event rules discussion Content information for participants
Event Rotation
The original “Reach for the Stars” event has been split into two separate, rotating events. Each topic has a consecutive two-year run.1. Reach for the Stars (2008-2009)2. The Solar System (2010-2011)3. Pattern is then repeated …
Motivation for splitting the event was to spread the immense body of accumulated knowledge over a longer period of time.
Deviation from the Original“Reach for the Stars” Event
“Reach for the Stars” is now solely a “stars” event and, as such, will no longer include:
1. location and identification of planets on star charts, etc.
2. the term “zodiac” to avoid the pseudo-science of astrology.
3. or references to asterisms.
Parent/Community Volunteers
With the ever-increasing responsibilities associated with teaching, seek out volunteers to coach as many of the events as possible.
Parents, especially, like their children to be successful and cherish opportunities to play a larger role in their lives.
Parent/Community Volunteers
Should you choose to pass this event on to a volunteer, provide him/her with a copy of this PowerPoint presentation. It will provide guidance and direction for individuals unfamiliar with the Science Olympiad.
Check with the volunteer frequently to provide assistance and check on participant progress.
Keep Informed!
Encourage your Science Olympiad participants to visit the NSO Clarifications Page for recent updates. The URL for clarifications is linked to: http://www.soinc.org The menu item is “FAQ.”
It is crucial that this be done at least one week prior to each competition.
Only those clarifications posted on the Official NSO website and direct information from your own State and Regional Directors are valid!
Description
Students will demonstrate an understand-ing and basic knowledge of stellar properties, stellar evolution, open and globular clusters, and spiral, elliptical and irregular galaxies.
Event Parameters
The only resource permitted is one 8.5” x 11.5” two-sided page of notes containing information in any form from any source.
Suggested information as to what to include on the resource sheet follows. Participants may think of other items they believe might also be helpful.
Event Parameters
Suggested information to include on the resource sheet for each star:
a. Name. Example. Solb. Classification. G2Vc. Evolutionary stage. Main sequenced. Constellatione. RA/Declination, i.e. locationf. Unique characteristics, if any
Event Parameters
Suggested information to include on the resource sheet for each Deep Sky Object:
a. Nameb. Constellationc. Messier number, i.e. M1, M13, etc.d. Kind of object: SNR, Globular cluster,
etc.e. RA/Declination (for location)f. Thumbnail imageg. Unique characteristics
Event Parameters –Suggested Resource Materials
H-R Diagram including the names of the stars Stages in the life cycle of a mid-sized star Stages in the life cycle of a massive star Characteristics of open & globular clusters Characteristics of spiral, elliptical and irregular galaxies Diagram of the Sun displaying its features and a brief
description of each Labeled diagrams of the constellations including the
stars and deep sky objects within them Glossary of frequently used and confusing terms
The Competition
The event is divided into two parts1. Notes may be used in both
2. Parts I and II may be combined
The Competition: Star Charts, Portable Star Labs, etc.
Participants will be asked to identify some or all of the stars, constellations and deep sky objects included in the official stars and objects list as they appear on star charts, H-R diagrams, portable star labs, photos, slides or in planetariums.
The Competition: List with Key Note: Constellations are underlined; stars
are bold face; and deep sky objects are italicized.
Objects preceded by an asterisk are new for 2009.
Participants must provide their own clipboards and red-filtered flashlights, unless officially notified otherwise.
The Competition
Part I: Coaching suggestions – Star Chartsa. Discuss the keys that generally accompany star charts.b. Compare right ascension and declination to latitude
and longitudec. Instruct participants on how to locate stars and deep sky objects using R.A./Declination.d. Make certain participants are able to properly record the R.A./Declination (R.A. following by declination)
The Competition: Stellar Evolution Participants should know the current stage
of each star and deep sky object Frequent observations of the night sky to
note star colors, relative positions to “neighboring” stars, and the seasons during which each is visible.
The Competition: Sky Observations
Associate the various stars and objects with the constellations in which they are found.
It is sometimes easiest to first locate the constellation and then the stars and objects that are in the constellation.
At other times it is easiest to first locate a star and then its constellation.
The Competition: Sky Observations
Stars are seasonal! This means that only between a quarter and a third of the stars on the list may be visible on any given (clear) night.
A few very late observations (after midnight) reveals stars that are not visible earlier in the evening. (Adult supervision required.)
Stars
Stars and objects in the list were selected to represent the various stages in the lives of stars.
The Large and Small Magellanic Clouds have been included in the list Science Olympiad list as there are no comparable objects visible to the unaided eye in the Northern skies.
Constellations
Constellations have been included1. for historical purposes,2. for ease of locating specific objects in the sky,3. and for those individuals fascinated with their mythological and literary history.
Participants should be aware that constellations are imaginary groupings of stars with limited scientific significance, except for astronomical reference, i.e. Cas A, Sgr A*, etc.
Part II: Hands-On orInterpretive Tasks
Participants will be asked to complete one or more hands-on or interpretive tasks selected from the following topics:
1. Characteristics of the Sun as an average-size star
2. Spectral classification of stars
3. Evolutionary stages of stars, open and globular clusters, and galaxies
National ScienceEducational Standards
The NSES have been included in all E-S Event rules to:
1. Align the events with the NSES
2. Make it easier for those teachers who wish to justify E-S event content within their curriculum
Spectral Classification
Standard means of recording the classification of a star. Example: The Sun is a G2V star.
1. Letter of class – O, B, A, F, G, K, M
2. Temperature number – 0 to 9
3. Luminosity category – Ia, Ib, II, III, IV, V, VI, VII
Spectral Classification
Each star class is divided into 10 sub-classes, ranging from 0 (hottest) to 9 (coolest).
Spectral Classification
Luminosity Classes are designated by Roman numerals I thru VII, in order of decreasing luminosity:
1. Ia - most luminous supergiants2. Ib - less luminous supergiants3. II - luminous giants 4. III - normal giants5. IV - subgiants6. V - main sequence and dwarfs 7. VI - subdwarfs8. VII - white dwarfs
Spectral Classification
Color of a star is dependent upon on its temperature 1. Red Stars are Cooler 2. Blue Stars are Hotter 3. (Very distant, dim stars appear white to the eye.)
Spectral Classification 1. Classify stars by their spectral lines 2. Spectral differences are due mostly to temperature, not
composition. Spectral Sequence (Temperature Sequence): O B A F G
K M L T
Spectral Classification
The traditional mnemonics for remembering the spectral types are based on the old Harvard OBAFGKM system.
1. Harvard (1920s): Oh Be A Fine Girl, Kiss Me
2. Berkeley (late `60s): Oh Buy A Fine Green Kilo Man
3. Caltech (late `70s): On Bad Afternoons Fermented Grapes Kept Mrs. (Richard Nixon Smiling)
Coaching Resources:Stellar Bingo
Objective: To provide a fun, hands-on experience for participants to become familiar with stellar images representing a variety of stages in the lives of stars.
This activity is available on the clinic’s website. If your kids enjoy the activity, it’s best to download it a.s.a.p. as it won’t be available forever.
Coaching Resources:Stellar Bingo
In a Bingo-type format, each player is given a card with numbered images.
When a clue is read, players attempt to match the clue with the photos on his/her card.
If a matching image appears on the card, a marker is placed on that image.
Discussion may follow as needed and adjustments made, add or remove marker.
Coaching Resources:Star Clues
Introduces students to the H-R Diagram through a challenging activity requiring students to complete a chart from a series of clues.
http://www.tufts.edu/as/wright_center/products/sci_olympiad/sci_olympiad_astro.html
Scroll down to: • Astronomy (Practice Activity - C Division)
Ignore the C-Division recommendation as H-R Diagrams are now a part of B-Division also.
The following slides provide a preview of this activity.
StarName
SpectralType
LuminosityClass
H-R Type Distance AbsoluteMagnitude
ApparentMagnitude
Color
Sirius V
Canopus F Ia -0.72
Arcturus +0.2 -0.04
Aldebaran Far
Spica Blue
Antares -5.2 +1.0
Deneb A Ia
Regulus B MainSequence
-0.3
Altair A +0.8
Capella G Giant +0.4
Rigel Supergiant +0.1
Sample Clue
Clue Card Information:
The absolute magnitudes of Regulus and Aldebaran are of equal value.
The chart provides the absolute magnitude for Regulus, but not for Aldebaran.
The clue card states that the absolute magnitude of these two stars are the same.
Therefore you know and may enter the absolute magnitude of Aldebaran on the chart.
StarName
SpectralType
LuminosityClass
H-R Type Distance AbsoluteMagnitude
ApparentMagnitude
Color
Sirius V
Canopus F Ia -0.72
Arcturus +0.2 -0.04
Aldebaran Far -0.3
Spica Blue
Antares -5.2 +1.0
Deneb A Ia
Regulus B MainSequence
-0.3
Altair A +0.8
Capella G Giant +0.4
Rigel Supergiant +0.1
Coaching Resources:Star Clues
The cards are shuffled and read at random. Sometimes the clue provided on a card is helpful;
sometimes it is not. If the information on the card is relevant, the information
may be entered on the chart and the card set aside. If the information is not relevant at this time, the card is
placed at the bottom of the deck. The information on all cards will eventually provide useful information for completing the chart.
The next card is then drawn.
StarName
SpectralType
LuminosityClass
H-R Type Distance AbsoluteMagnitude
ApparentMagnitude
Color
Sirius A V MainSequence
Near +1.5 -1.5 White
Canopus F Ia Supergiant Far -2.5 -0.72 PaleYellow
Arcturus K III Giant Medium +0.2 -0.04 Orange
Aldebaran K III Giant Far -0.3 +0.9 Orange
Spica B V MainSequence
Far -3.2 +1.0 Blue
Antares M Ib Supergiant Far -5.2 +1.0 Coral
Deneb A Ia Supergiant Far -7.2 +1.3 White
Regulus B V MainSequence
Far -0.3 +1.4 Blue
Altair A V MainSequence
Near +2.3 +0.8 White
Capella G III Giant Medium +0.4 +0.08 Gold
Rigel B 1a Supergiant Far -8.1 +0.1 Blue
Coaching Resources:Practice Exam
This exam is available on the clinic website. It utilizes the Stellar Cycle Cards distributed during this session and is also available at no cost to educators from the Chandra X-ray Center. To request one or more sets of cards, visit: http://chandra.harvard.edu/edu/formal/stellar_cycle/
Coaching Resources:STELLAR JOURNEY: The Game
STELLAR JOURNEY: The Game presents a simulation of star life from birth through death. The game is a very hands-on, exciting, and relevant to Reach for the Stars and Astronomy events of the SO. To learn more, visit:
www.otherworlds-edu.com
Request a Free Stellar Evolution Poster from the Chandra X-ray Center
Request two posters – one to post the front of the poster (shown) and one to post for the information on the back
http://chandra.harvard.edu/edu/formal/stellar_ev/
Coaching Resources:The Game of SPACE
The Game of SPACE quizzes players on their knowledge of Stars, Planets, Astronomy, Constellations and Exploration.
New 2008 edition is now available.
www.otherworlds-edu.com
Coaching Resources:Internet
Discuss the importance of consulting only “reliable” web sites when surfing the web.
Ask students to limit their searches to legitimate organizations: NASA, NOAA, USGS, colleges and other trustworthy public and private institutions, etc. Almost any information students may require is quite likely to be found on these sites.
Does the organization appear to have an agenda? Example: Is the “global warming” debate really over? If a site fails this test, ask students to continue their search elsewhere.
Discuss questioning information that appears at odds with information obtained from legitimate sites. If someone has a “gut-feeling” that something being said is a bit “far-out,” it just may be.
Coaching Resources:Internet
Previously administered Astronomy and Reach for the Stars exams have been posted on The Wright Center Website. Many of the C-Division exams are now relevant to the B-Division event. Use “Wright Center Science Olympiad” as the key phrase. Click on the SO Logo on the left of the page to be taken to the site.
Coaching Resources:Internet
Excellent information on Stellar Evolution may be found on the Chandra X-ray Center website. Visit:
http://chandra.harvard.edu/edu/formal/stellar_ev/story/
Coaching Resources:Internet
An article on stellar evolution appearing in the World Book Encyclopedia, written in cooperation with NASA, may be found at:
http://www.nasa.gov/worldbook/star_worldbook.html
Test-Taking Strategies
Listen carefully to all instructions provided at the beginning of the session.
Read all information included on the exam. Ignore any and all comments regarding how well
or how poorly other members of your team have performed during previous events.
Decide upon roles for you and your partner well in advance of the competition.
Stellar Evolution of Stars
Formation in a stellar nursery … through birth … each life stage … and final product – (white dwarf, neutron star, black hole).
Stellar Evolution of Stars
Participants may anticipate having to interpret one or more charts or graphs.
The following two slides are examples of the kind of charts or graphs a supervisor might include.
Participants could “brain storm” several questions that might be asked about these particular charts and graphs.
Star Clusters: Definition
Gravitationally-bound collection of stars that formed from the same gas cloud.
Open Clusters
1. Contain a few (typically tens to thousands of) young stars
2. Individual stars are easily resolved
Image: WIYN Telescope, Kitt Peak
Open Clusters
3. Open clusters are collections of hot, recently formed stars found preferentially in the spiral arms of the galaxy.
4. Stars within open clusters eventually disperse.Credit: AURA, NOAO, NSF
Globular Clusters
1. Are found in the haloes of galaxies2. Contain from tens of thousands to millions of ancient stars crowded into a more or less spherical volume of space.
Image: Hubble Space Telescope
Globular Clusters
3. Their central density is sufficiently high that individual stars cannot be resolved from earth-based telescopes
Image: Sonoita Observatories
Spiral Galaxies
1. Disk-shaped, usually with a bulge at the center and arms spiraling outwards
2. Tend to contain more middle-aged stars along with clouds of gas and dust
The spiral galaxy NGC 1309
Spiral Galaxies
Image courtesy Richard Crisp
3. Spiral galaxies contain large concentrations of gas and dust.
4. The spiral arms are waves of star formation swirling around the galaxy.
5. New stars are hot and bright. They light up the gas and dust in the arms.
Elliptical Galaxies
1. Contain older stars and very little gas and dust
2. Can be different shapes ranging from round, to flattened, elongated spheres.
3.Orbits of stars within elliptical galaxies are in random directions
NOAO/AURA/NSF
Elliptical Galaxies
4. Contain modest amounts of cool and warm gas, though not as much as found in spiral galaxies.
5. There are generally not enough gases to support much star formation.
NOAO/AURO/NSF
Galactic Types & Structure
Irregular galaxies
1. Poorly-defined structures
2. Have lots of young stars, dust and gas.
3.Show evidence of extensive star formation
Image courtesy of Richard Crisp.
Constellation: Andromeda
Deep Sky Object: Andromeda Galaxy M-31
Constellation: *Aquarius
Deep Sky Object: *Helix Nebula
The Helix Nebula is one of the closest and apparently one of the largest planetary nebulae known.
Constellation: Aquila
Star: Altair Spectral Type: A7V Main Sequence
Constellation: Auriga
Star: Capella Spectral Type: G8 III Red Giant
Constellation: Bootes
Star: Arcturus – Spectral Type: K2 III Red Giant
Brightest star in the Northern Hemisphere
Constellation: Cancer
Deep Sky Object:
M44 Beehive
Tom Bash and John Fox/Adam Block/NOAO/AURA/NSF
Constellation: Canes Venatici
Deep Sky Object:
M51 Whirlpool Galaxy
Constellation: Canis Major
Star: Sirius A Spectral Type: A1 V Main Sequence
Star: *Sirius B. Not visible to the unaided eye due to its close, extremely bright, companion, Sirius A
Constellation: Canis Minor
Star: Procyon Spectral Type: F5 IV Subgiant
Constellation: Cassiopeia
Deep Sky Object
Tycho’s SNR
Constellation: Cassiopeia
Deep Sky Object
Cas A - SNR
Constellation: *Cygnus
Star: *Deneb (tail) Spectral Type: A2 Ia Supergiant Deep Sky Object (SNR)
*Veil Nebula (red)
Constellation: Gemini
Star: Castor (top) Spectral Type: A1 V Main Sequence
Star: Pollux (bottom) Spectral Type: K0 III Giant
Constellation: Hercules
M13 Globular Cluster
©Richard Crisp
Constellation: *Leo
Star: *Regulus Spectral Type: B7 V Main Sequence
Star: *Wolf 359 (red) Spectral Type: M5.8 Main Sequence –
Red Dwarf
Constellation: Lyra
Star: Vega
Spectral Type: A0 V
Main sequence, Blue
Deep Sky Object: Ring Nebula – M57 (red)
MILKY WAY GALAXYCredit & Copyright: Richard Payne (Arizona Astrophotography)
Constellation: Orion
Star: Betelgeuse (upper)
Spectral Type: M2 Ib
Red supergiant
Star: Rigel (lower)
Spectral Type: B8 Ia
Blue Supergiant
M42 Orion Nebula (red)
Constellation: Orion
M42 Orion Nebula
Constellation: Orion*Trapezium (Within Orion Nebula)
Constellation: PerseusStar: Algol
Spectral Types:
B8 V & G5 IV
Star A is separated from close companion B by less than a tenth (0.062) of the Earth-Sun distance (AU). Dimmer Star B partially eclipses Star A every 2.9 days and loses gas in a "star stream" that impacts Star A before bouncing back out to create a "transient accretion annulus" around Star A
Constellation: Sagittarius
Deep Sky Object:Sgr A*
Photo: Chandra X-ray Observatory
Constellation: *Scorpius
Star: Antares Spectral Type: M1 Ib Supergiant
Deep Sky Object:*M6 Butterfly Cluster (red)
Credit: AURA, NOAO, NSF
Constellation: Taurus
Star: Aldebaran Spectral Type: K5 III Orange-Red Giant
Star Cluster: Hyades (red)
Star Cluster: Pleiades (green)
Constellation: Taurus
Deep Sky Object - Star Cluster: M45 Pleiades (upper image)
Deep Sky Object SNR: M1Crab Nebula (lower image)
Constellation: Tucana
Deep Sky Object: Small Magellanic Cloud (NASA/ESA)
Constellation: Ursa Minor
Star: Polaris Spectral Type: F8 Ib Supergiant
A Cepheid Variable
Constellation: Virgo
Star: Spica Spectral Type: B1 V Main Sequence
Latin for “Ear of Wheat” held in the maiden’s hand.
Constellation: Vulpecula
Deep Sky Object: M27 Dumbbell Nebula