Station

Star system
Power
-
Station distance
6,190 Ls
Planet
Leleng Musu BC 1 Odyssey
Landing pad
Large
Station type
Surface Port

Station services
Commodity marketOutfittingRearmRefuelRepairShipyard

Black marketContactsFleet carrier administrationFleet carrier servicesFleet carrier vendorInterstellar factorsMaterial traderPower contactRedemption officeSearch and rescueTechnology brokerUniversal CartographicsVendorsWorkshop

BartenderConcourseCrew loungeFrontline SolutionsMissionsPioneer SuppliesTuningVista Genomics


Economy
Refinery
Wealth
Population
Government
Patronage
Allegiance
Independent

Station update
17 Nov 2024, 10:22pm
Location update
17 Nov 2024, 10:22pm
Market update
17 Nov 2024, 10:22pm
Shipyard update
Outfitting update
17 Nov 2024, 10:22pm

Galpedia

Henrietta Swan Leavitt

Henrietta Swan Leavitt (July 4, 1868 – December 12, 1921) was an American astronomer who discovered the relation between the luminosity and the period of Cepheid variable stars. A graduate of Radcliffe College, Leavitt started working at the Harvard College Observatory as a "computer" in 1893, examining photographic plates in order to measure and catalog the brightness of stars. Though she received little recognition in her lifetime, it was her discovery that first allowed astronomers to measure the distance between the Earth and faraway galaxies. She explained her discovery: “A straight line can readily be drawn among each of the two series of points corresponding to maxima and minima, thus showing that there is a simple relation between the brightness of the variables and their periods.” After Leavitt's death, Edwin Hubble used the luminosity-period relation for Cepheids together with spectral shifts first measured by fellow astronomer Vesto Slipher at Lowell Observatory to determine that the universe is expanding (see Hubble's law).



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