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Hubble Measures Deflection of Starlight by a Foreground Object

Hubble Measures Deflection of Starlight by a Foreground Object

How Gravity Can Bend Starlight

This illustration reveals how the gravity of a white dwarf star warps space and bends the light of a distant star behind it.

White dwarfs are the burned-out remnants of normal stars. The Hubble Space Telescope captured images of the dead star, called Stein 2051 B, as it passed in front of a background star. During the close alignment, Stein 2051 B deflected the starlight, which appeared offset by about 2 milliarcseconds from its actual position. This deviation is so small that it is equivalent to observing an ant crawl across the surface of a quarter from 1,500 miles away. From this measurement, astronomers calculated that the white dwarf's mass is roughly 68 percent of the sun's mass.

Stein 2051 B resides 17 light-years from Earth. The background star is about 5,000 light-years away. The white dwarf is named for its discoverer, Dutch Roman Catholic priest and astronomer Johan Stein.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    04h 31m 13s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +58° 58' 41"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Camelopardalis
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    17 light-years (5.5 parsecs)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Stein 2051 B, WD 0426+588
  • Object Description
    Object DescriptionThe type of astronomical object.
    White dwarf star
  • Release Date
    June 7, 2017
  • Science Release
    Hubble Astronomers Develop a New Use for a Century-Old Relativity Experiment to Measure a White Dwarf’s Mass
  • Credit
    NASA, ESA, and A. Feild (STScI)

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov