0
The Distance Ladder
                       LACC §18.3, 19.1, 19.5

              • Within the Solar System
              •...
Stellar Parallax
           (Distance Ladder)




                 http://www.astro.umd.edu/educationalresources/astro/spr...
Stellar Parallax: Hipparcos
      Hipparcos is an acronym for HIgh Precision PARallax COllecting
      Satellite. Appropri...
The Closest Stars




                           http://calgary.rasc.ca/stellarmagnitudes.htm

Thursday, April 22, 2010   ...
HR Diagram




       http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_hrintro.html
Thursday, ...
Main Sequence Fitting
               (a type of Standard Candle)
                                                         ...
Variable Stars
               (a type of Standard Candle)




                      http://www.mhhe.com/physsci/astronomy/...
Variable Stars
               (a type of Standard Candle)
                                 disregard the colors in these d...
The Distance Ladder
                       LACC §18.3, 19.1, 19.5
              • Within the Solar System: Radar Ranging
 ...
LACC HW: Franknoi, Morrison, and
                Wolff, Voyages Through the Universe,
                               3rd e...
The Interstellar Medium
                       LACC §18.3, 19.1, 19.5

              • Nebulae
              • Dust
      ...
Where did all the stars go? What used
      to be considered a hole in the sky is
                                        ...
HII Regions




                                  M42 Orion Nebula and NGC1977
                           Note: HII region...
Orion: Visible vs. Infrared


           Betelgeuse




              Orion
              Nebula
                         ...
Planetary Nebula
                             aka The Saturn Nebula




          http://www.ucl.ac.uk/star/research/stell...
Reflection Nebula

                                                                           Note: reflection
             ...
Supernova Remnant




     SN 1006 Supernova Remnant
     A new star, likely the brightest supernova in recorded human his...
The Local Bubble




                                   http://www.sslmit.unibo.it/zat/images/
                           ...
Dust Grains




           A cosmic dust cloud sprawls across a rich
            field of stars in this gorgeous wide field
...
Dust Grains




            The grains appear to be loose conglomerations of
             smaller specks of material, whic...
The Interstellar Medium
                       LACC §18.3, 19.1, 19.5
      • Nebulae: Dark Dust Clouds (aka Molecular Clo...
LACC HW: Franknoi, Morrison, and
                Wolff, Voyages Through the Universe,
                               3rd e...
Upcoming SlideShare
Loading in...5
×

A1 17 Ism

1,133

Published on

Miller's Astronomy 1 lecture notes on the Interstellar Medium

Published in: Education, Technology, Spiritual
0 Comments
1 Like
Statistics
Notes
  • Be the first to comment

No Downloads
Views
Total Views
1,133
On Slideshare
0
From Embeds
0
Number of Embeds
1
Actions
Shares
0
Downloads
70
Comments
0
Likes
1
Embeds 0
No embeds

No notes for slide

Transcript of "A1 17 Ism"

  1. 1. The Distance Ladder LACC §18.3, 19.1, 19.5 • Within the Solar System • Within the Galaxy • Within the Universe An attempt to answer the “big questions”: What is out there? How big is the universe? Thursday, April 22, 2010 1
  2. 2. Stellar Parallax (Distance Ladder) http://www.astro.umd.edu/educationalresources/astro/sprop/parallax.html Thursday, April 22, 2010 2
  3. 3. Stellar Parallax: Hipparcos Hipparcos is an acronym for HIgh Precision PARallax COllecting Satellite. Appropriately the proununciation is also very close to Hipparchus, the name of a Greek astronomer who lived from 190 to 120 BC. By measuring the position of the Moon against the stars, Hipparchus was able to determine the Moon's parallax and thus its distance from the Earth. He also made the first accurate star map which lead to the discovery, when compared with other data from his predecessors, that the Earth's poles rotate in the sky, a phenomenon referred to as the precession of the equinoxes. ...distances accurate to ... 10%. For a typical measurement accuracy of 1 milliarcsec, this will mean stars with parallaxes ... 10 milliarcsec, i.e. stars within ... 100 pc of the Sun. http://www.rssd.esa.int/index.php?project=HIPPARCOS&page=FAQ Thursday, April 22, 2010 3
  4. 4. The Closest Stars http://calgary.rasc.ca/stellarmagnitudes.htm Thursday, April 22, 2010 4
  5. 5. HR Diagram http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_hrintro.html Thursday, April 22, 2010 5
  6. 6. Main Sequence Fitting (a type of Standard Candle) If you have a cluster of stars of unknown distance, you can compare how bright the stars on its main sequence appear with how bright the stars in a cluster of known distance appear. In the example above, the stars in the Pleiades (an open cluster) are 7.5 times dimmer than the stars in the Hyades (also an open cluster), and so must be further away.You can use the inverse-square law (apparent brightness = true luminosity / 4 pi R2) to show that the Pleiades is sqrt(7.5) times further away than the Hyades. http://www.bramboroson.com/astro/apr29.html Thursday, April 22, 2010 6
  7. 7. Variable Stars (a type of Standard Candle) http://www.mhhe.com/physsci/astronomy/arny/instructor/graphics/ ch13/1312.jpg Thursday, April 22, 2010 7
  8. 8. Variable Stars (a type of Standard Candle) disregard the colors in these diagrams http://abyss.uoregon.edu/~js/ http://astronomy.nmsu.edu/ ast122/lectures/lec15.html tharriso/ast110/class22.html Thursday, April 22, 2010 8
  9. 9. The Distance Ladder LACC §18.3, 19.1, 19.5 • Within the Solar System: Radar Ranging • Within The Galaxy: Stellar Parallax, Main- Sequence Fitting (aka Spectroscopic Parallax), Cepheid Variable • Within the Universe: Tully-Fisher Relation, Type Ia Supernova, Brightest Cluster Galaxy, Hubble’s Law An attempt to answer the “big questions”: What is out there? How big is the universe? Thursday, April 22, 2010 9
  10. 10. LACC HW: Franknoi, Morrison, and Wolff, Voyages Through the Universe, 3rd ed. • Ch 18, pp. 413: 5 (choose your answers from the following: standard candle using main sequence fitting, radar ranging, standard candle using RR Lyrae and Cepheids’ period luminosity relation, stellar parallax). • Ch 20: Tutorial Quizzes accessible from: www.brookscole.com/cgi-brookscole/course_products_bc.pl? http:// fid=M20b&product_isbn_issn=9780495017899&discipline_number=19 Due at the beginning of the next class period. Thursday, April 22, 2010 10
  11. 11. The Interstellar Medium LACC §18.3, 19.1, 19.5 • Nebulae • Dust • Gas An attempt to answer the “big questions”: What is out there? How big is the universe? Thursday, April 22, 2010 11
  12. 12. Where did all the stars go? What used to be considered a hole in the sky is Molecular Cloud now known to astronomers as a dark molecular cloud. Here, a high concentration of dust and molecular gas absorb practically all the visible light emitted from background stars. The eerily dark surroundings help make the interiors of molecular clouds some of the coldest and most isolated places in the universe. One of the most notable of these dark absorption nebulae is a cloud toward the constellation Ophiuchus known as Barnard 68, pictured above. That no stars are visible in the center indicates that Barnard 68 is relatively nearby, with measurements placing it about 500 light-years away and half a light-year across. It is not http://apod.nasa.gov/apod/ap041219.html known exactly how molecular clouds like Barnard 68 form, but it is known that these clouds are themselves likely Note: molecular clouds are places for new stars to form. It is dark in color. Why? possible to look right through the cloud in infrared light. Thursday, April 22, 2010 12
  13. 13. HII Regions M42 Orion Nebula and NGC1977 Note: HII regions are reddish in color. Why? http://autostarsuite.net/photos/snoleopard/picture3566.aspx Thursday, April 22, 2010 13
  14. 14. Orion: Visible vs. Infrared Betelgeuse Orion Nebula Rigel http://www.compadre.org/informal/features/featureSummary.cfm?FID=642 Thursday, April 22, 2010 14
  15. 15. Planetary Nebula aka The Saturn Nebula http://www.ucl.ac.uk/star/research/stellarenvironment/cieresearch/planetarynebulae Thursday, April 22, 2010 15
  16. 16. Reflection Nebula Note: reflection nebula are bluish in color. Why? Unspeakable beauty and unimaginable bedlam can be found together in the Trifid Nebula. Also known as M20, this photogenic nebula is visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. The red-glowing gas results from high-energy starlight striking interstellar hydrogen gas. The dark dust filaments that lace M20 were created in the atmospheres of cool giant stars and in the debris from supernovae explosions. Which bright young stars light up the blue reflection nebula is still being investigated. The light from M20 we see today left perhaps 3000 years ago, although the exact distance remains unknown. Light takes about 50 years to cross M20. http://apod.nasa.gov/apod/ap070813.html Thursday, April 22, 2010 16
  17. 17. Supernova Remnant SN 1006 Supernova Remnant A new star, likely the brightest supernova in recorded human history, lit up planet Earth's sky in the year 1006 AD. The expanding debris cloud from the stellar explosion, found in the southerly constellation of Lupus, still puts on a cosmic light show across the electromagnetic spectrum. In fact, this composite view includes X-ray data in blue from the Chandra Observatory, optical data in yellowish hues, and radio image data in red. Now known as the SN 1006 supernova remnant, the debris cloud appears to be about 60 light-years across and is understood to represent the remains of a white dwarf star.... Because the distance to the supernova remnant is about 7,000 light-years, that explosion actually happened 7,000 years before the light reached Earth in 1006. http://apod.nasa.gov/apod/ap080704.html Thursday, April 22, 2010 17
  18. 18. The Local Bubble http://www.sslmit.unibo.it/zat/images/ cartography/M-Way_2.htm Thursday, April 22, 2010 18
  19. 19. Dust Grains A cosmic dust cloud sprawls across a rich field of stars in this gorgeous wide field Very small solid particles or "dust grains"; telescopic vista looking toward Corona smoke-like. These absorb and redden Australis, the Southern Crown. Probably light passing through them. less than 500 light-years away and Absorption by dust creates "dark clouds" effectively blocking light from more seen against bright sources such as the distant, background stars in the Milky Way, Milky Way. the densest part of the dust cloud is about 8 light-years long. http://www.astro.virginia.edu/ class/oconnell/astr121/ http://antwrp.gsfc.nasa.gov/ guide11.html apod/ap040715.html Thursday, April 22, 2010 19
  20. 20. Dust Grains The grains appear to be loose conglomerations of smaller specks of material, which stuck together after bumping into each other in the depths of space. http://spiff.rit.edu/classes/phys230/lectures/ism_dust/ism_dust.html Thursday, April 22, 2010 20
  21. 21. The Interstellar Medium LACC §18.3, 19.1, 19.5 • Nebulae: Dark Dust Clouds (aka Molecular Clouds), HII Regions (e.g. star-forming regions, planetary nebulae; HII emission line), Reflection Nebulae (reflection off dust), Supernova Remnants • Dust: 1 grain / 1012 atoms; silicates, carbon, ices • Gas: 90% H, 9% He, 1% heavier (by number); 1 atom / cm3 (1000 / cm3 is an excellent laboratory vacuum), 100 Kelvin (but varies) An attempt to answer the “big questions”: What is out there? How big is the universe? Thursday, April 22, 2010 21
  22. 22. LACC HW: Franknoi, Morrison, and Wolff, Voyages Through the Universe, 3rd ed. • Ch 19, p. 435: 13, 14. • Ch 21: Tutorial Quizzes accessible from: http:// www.brookscole.com/cgi-brookscole/course_products_bc.pl? fid=M20b&product_isbn_issn=9780495017899&discipline_number=19 Due at the beginning of the next class period. Thursday, April 22, 2010 22
  1. A particular slide catching your eye?

    Clipping is a handy way to collect important slides you want to go back to later.

×