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Measure distance of celestial bodies
이주원 정지혁 조완
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https://en.wikipedia.org/wiki/Local_Group
Tarenghi, Massimo, et al. "The Hercules supercluster. I-Basic data." The Astrophysical Journal 234 (1979):
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Measurement methods Standard candles Statistic method
Cepheid variables Supernovae Statistic method Main sequence fitting Tully-Fisher relation Surface Brightness fluctuation
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Cepheid Variables 𝑀=−2.76 𝑙𝑜𝑔𝑃−1 −4.16 Surface atoms ionized
Transparency increase Temperature increase Temperature decrease Transparency decrease Surface atoms unionized 𝑀=−2.76 𝑙𝑜𝑔𝑃−1 −4.16
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Type Ia supernovae 𝑀≈−17.5
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Main sequence fitting
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Tully-Fisher relation
𝑀=−9.5 𝑙𝑜𝑔 𝑊 𝑅 −2.5 −21.67 𝑊 𝑅 is 𝑘𝑚/𝑠 unit Aaronson, M., et al. "A catalog of infrared magnitudes and HI velocity widths for nearby galaxies." The Astrophysical Journal Supplement Series 50 (1982):
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Surface brightness fluctuation
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New measurement methods
Electromagnetic wave signal (EM wave) gravitational-wave & multi-messenger astronomy Gravitational wave signal (GW)
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Standard Siren Standard candle Standard Siren
The two objects rapidly spiral together Cepheid variables Supernovae
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Principle of Standard Siren
Two-neutron-star binary system, 𝑓 100 Distance 𝑟 100 Angular momentum axis Angle ι elliptical polarization of GW Earth 𝑟 100 = 7.8 𝑓 100 −2 ( ℎ× 𝜏) −1 (ℎ: r.m.s. value of amplitude averaged over orientations)
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LIGO’s measurement of H0
d= − Mpc 𝐻 0 = − km s−1 Mpc−1 LIGO Scientific Collaboration et al., A gravitational-wave standard siren measurement of the Hubble constant, Nature 551, 85 (2017).
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Reference Zeilik, Michael, and Elske van Panhuys Smith. Introductory astronomy and astrophysics. Philadelphia: Saunders College Pub., c nd ed. (1987). Karttunen, Hannu, et al., eds. Fundamental astronomy. Springer, 2016. LIGO Scientific Collaboration et al., A gravitational-wave standard siren measurement of the Hubble constant, Nature 551, 85 (2017). Bernard F. Schutz , Determining the Hubble constant from gravitational wave observations ,Nature 323, 25 (1986)
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