🌌 Astronomy Evening at Valley View Hot Springs

Tour of the Universe with the 20" PlaneWave Telescope


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We often dream of travelling the world and seeing its many wonders, but few people have the time or money to see much of it. Even though the distances are much greater, astronomy is more accessible than geography: half the universe is visible on any clear evening, and you can look at most of it in one night.

The universe is easy to observe, dynamic, deeply related to our existance (the hopfully-familiar story of the big bang and creation and supernovae creating the elements that our bodies are made of.)

See the Moon, constellations, stars, planets, Earth satellites, and more via the naked eye, binoculars and a small telescope. For your mind’s eye we’ll point out newly-discovered solar systems, black holes, X-ray sources, the Hubble Deep Field and bask (as always :-) in the presence of the 2.73 degree K cosmic microwave background radiation from the Big Bang.

Cosmic Distance Ladder (Orders of Magnitude)

8 factors of 1000 in distance → 24 orders of magnitude!
48 orders of magnitude in brightness!!

Distance Scientific Notation Scale Example / Note
30 m 30 × 10⁰ m 100 ft [something at “1st mag” and “12th mag”]
30 km 30 × 10³ m 20 miles Denver
400 km 400 × 10³ m 500 km International Space Station close pass
3 Mm 3 × 10⁶ m 3000 km Boston, is a candle about 11th mag?
42.2 Mm 42 × 10⁶ m 24 hr orbit Geosynchronous satellite orbit
384 Mm 384 × 10⁶ m 384,000 km Moon
56 Gm 56 × 10⁹ m 0.37 AU Mars - closest (Venus: 0.27 AU = 40 Gm)
150 Gm 150 × 10⁹ m 1 AU Sun
1.4 Tm 1.4 × 10¹² m 9.5 AU Saturn
5.9 Tm 5.9 × 10¹² m 39.5 AU Pluto
10 Tm 30 × 10¹² m — Kuiper belt outer extents?
7 Pm 7 × 10¹⁵ m 50,000 AU Oort cloud
41 Pm 41 × 10¹⁵ m 4.40 ly Alpha Centauri - closest naked-eye star
222 Pm 222 × 10¹⁵ m 25.3 ly Vega
13 Em 13 × 10¹⁸ m 3000 ly Deneb
600 Em 600 × 10¹⁸ m 60 kly M54 - far side of our galaxy
22 Zm 22 × 10²¹ m 2.5 Mly Andromeda galaxy (M31)
110 Zm 110 × 10²¹ m 12 Mly M64 Black-eye Spiral Galaxy
600 Zm 600 × 10²¹ m 60–70 Mly M49, M87 in Virgo cluster, M77 in Cetus
19 Ym 19 × 10²⁴ m 1.9 Bly 3C273, the brightest quasar
170 Ym 170 × 10²⁴ m 13.7 Bly Edge of the visible universe (CMB, z=1086, 0.380 Myr)
75 Ym 75 × 10²⁴ m 7.5 Gly GRB 080319B in Bootes (furthest visible object, 30s flare mag 5.8, 2008-03-19) Wikipedia

1. Setting the Scene: Valley View’s Dark Sky


2. Our Telescope: Beyond Magic


3. How the Naked Eye Misleads Us

  1. Our cosmos is filled with galaxies.
  2. Light pollution is erasing stars.
  3. Stars move.
  4. Bright stars are unusual.
  5. Stars are often in systems.

4. Dynamic, 3D Sky


5. Galaxies per Field of View


6. Cosmic Highlights


7. Largest Structures


8. Scale of the Universe


Cosmic Distance Ladder (Orders of Magnitude)

8 factors of 1000 in distance → 24 orders of magnitude!
48 orders of magnitude in brightness!!

Distance Scientific Notation Scale Example / Note
30 m 30 × 10⁰ m 100 ft [something at “1st mag” and “12th mag”]
30 km 30 × 10³ m 20 miles Denver
400 km 400 × 10³ m 500 km International Space Station close pass
3 Mm 3 × 10⁶ m 3000 km Boston, is a candle about 11th mag?
42.2 Mm 42 × 10⁶ m 24 hr orbit Geosynchronous satellite orbit
384 Mm 384 × 10⁶ m 384,000 km Moon
56 Gm 56 × 10⁹ m 0.37 AU Mars - closest (Venus: 0.27 AU = 40 Gm)
150 Gm 150 × 10⁹ m 1 AU Sun
1.4 Tm 1.4 × 10¹² m 9.5 AU Saturn
5.9 Tm 5.9 × 10¹² m 39.5 AU Pluto
10 Tm 30 × 10¹² m — Kuiper belt outer extents?
7 Pm 7 × 10¹⁵ m 50,000 AU Oort cloud
41 Pm 41 × 10¹⁵ m 4.40 ly Alpha Centauri - closest naked-eye star
222 Pm 222 × 10¹⁵ m 25.3 ly Vega
13 Em 13 × 10¹⁸ m 3000 ly Deneb
600 Em 600 × 10¹⁸ m 60 kly M54 - far side of our galaxy
22 Zm 22 × 10²¹ m 2.5 Mly Andromeda galaxy (M31)
110 Zm 110 × 10²¹ m 12 Mly M64 Black-eye Spiral Galaxy
600 Zm 600 × 10²¹ m 60–70 Mly M49, M87 in Virgo cluster, M77 in Cetus
19 Ym 19 × 10²⁴ m 1.9 Bly 3C273, the brightest quasar
170 Ym 170 × 10²⁴ m 13.7 Bly Edge of the visible universe (CMB, z=1086, 0.380 Myr)
75 Ym 75 × 10²⁴ m 7.5 Gly GRB 080319B in Bootes (furthest visible object, 30s flare mag 5.8, 2008-03-19) Wikipedia

9. Closing Themes