6. consist of relatively low-density ionized hydrogen. (a) HI regions (b) H Il regions (c) protostar (d) protoplanetary disk (e) dark nebula 7. When passing through interstellar medium, light is and (a) shocked; fragmented (b) excited; ionized (c) dimmed; reddened (d) speeded up; then slowed down (e) emitted; blue-shifted
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consist of relatively low-density ionized hydrogen.
(a) HI regions
(b) H II regions
(c) protostar
(d) protoplanetary disk
(e) dark nebula
7.
When passing through interstellar medium, light is.
and
(a) shocked; fragmented
(b) excited; ionized
(c) dimmed; reddened
(d) speeded up; then slowed down
(e) emitted; blue-shifted"
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Step by step
Solved in 3 steps
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- A)The star 58 Eridani is a feint but naked-eye star similar to the Sun. Suppose that you are observing this star in the night sky without a telescope. Ignoring any interstellar extinction or atmospheric absorption, approximately how many photons per second arrive at your retina? Show all steps in calculation . B) The Mid-infared Instrument (MIRI , camera and spectrograph ) on the James Webb Space Telescope operates in the band 5-28 µm . For 58 Eridani , approximatley how many photons per second can be used by this instrument ? Assume that MIRI takes all the photons from the full JWST mirror . Show all steps in calcultation . Describe breifly two or three other factors which play a role in determining the sensetivitu of an instrument such as MIRI ?Which portion of the EM spectrum is best for understanding the giant Molecular Clouds from which stars are born? Far infrared GXUVIR a. FAR IR b. VISIBLE OC. NEAR IR Od. Molecular Clouds are not shown in any of them Oe. All show the clouds equally well Visible wwwwwwww GXUVR Near infrared. www GXUVIR38. Many RR Lyrae stars are found in open clusters in the plane of the galaxy. True False
- What evidence can you cite that the interstellar medium contains both gas and dust? (Select all that apply.) (1)The dust of the interstellar medium can be detected from the emission lines of elements heavier than iron. (2)The dust of the interstellar medium can be detected by the extinction of light from distant stars. (3)The dust of the interstellar medium can be detected by the scattering of blue light from distant or embedded objects. (4)The gas of the interstellar medium can be detected from the radiation of ultraviolet photons. (5)The gas of the interstellar medium can be detected from the radiation of photons of wavelength 21 cm. (6)The gas of the interstellar medium can be detected from the absorption lines present in the light from distant stars, which must be caused by a medium of a density and temperature other than that of the stars emitting the light.1. Distance to moon is about one quarter million miles, how much is that in km? m? 2. Distance to star Proxima Centauri is about 2.4 x 1013 miles, how much is that in ly? AU? pc? 3. Distance to Sun is 93 million miles, how much is that in ly? AU? pc?