Station

Star system
Station distance
40 Ls
Planet
Maridwyn A 3 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
Industrial
Wealth
Population
Government
Corporate
Allegiance
Federation
Minor faction

Station update
10 Nov 2024, 5:03pm
Location update
10 Nov 2024, 5:03pm
Market update
10 Nov 2024, 4:43pm
Shipyard update
Outfitting update
10 Nov 2024, 4:43pm

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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