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  2. Epsilon Eridani - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Eridani

    Today numbers from this catalogue are used with the prefix "Lalande", or "Lal". [50]) Lalande assigned Epsilon Eridani magnitude 3. [48] [49] Also in 1801 it was included in the catalogue of Johann Bode, in which about 17,000 stars were grouped into 102 constellations and numbered (Epsilon Eridani got the number 159 in the constellation ...

  3. UDF 423 - Wikipedia

    en.wikipedia.org/wiki/UDF_423

    UDF 423 is the spiral galaxy in the lower right quadrant of the Hubble Ultra Deep Field.. UDF 423 is the Hubble Ultra Deep Field (UDF) identifier for a distant spiral galaxy.

  4. Eris (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Eris_(dwarf_planet)

    Eris was discovered by the team of Mike Brown, Chad Trujillo, and David Rabinowitz [2] on January 5, 2005, from images taken on October 21, 2003. [31] The discovery was announced on July 29, 2005, the same day as Makemake and two days after Haumea, [32] due in part to events that would later lead to controversy about Haumea.

  5. DX Cancri - Wikipedia

    en.wikipedia.org/wiki/DX_Cancri

    DX Cancri is a variable star in the northern zodiac constellation of Cancer.With an apparent visual magnitude of 14.81, [3] it is much too faint to be seen with the naked eye. ...

  6. 17α-Estradiol - Wikipedia

    en.wikipedia.org/wiki/17α-estradiol

    17α-Estradiol (also known as 17α-E2, 17-epiestradiol, alfatradiol, or estra-1,3,5(10)-triene-3,17α-diol) is a minor and weak endogenous steroidal estrogen that is related to 17β-estradiol (better known simply as estradiol). [2]

  7. HR 7703 - Wikipedia

    en.wikipedia.org/wiki/HR_7703

    HR 7703 (Gliese 783, 279 G. Sagittarii) is a binary star system in the constellation of Sagittarius.The brighter component has an apparent visual magnitude of 5.31, [2] which means it is visible from suburban skies at night.

  8. WISE 0350−5658 - Wikipedia

    en.wikipedia.org/wiki/WISE_0350%E2%88%925658

    WISE 0350-5658 with unWISE. WISE 0350−5658 was discovered in 2012 by J. Davy Kirkpatrick and colleagues from data collected by the Wide-field Infrared Survey Explorer (WISE) in the infrared at a wavelength of 40 cm (16 in), whose mission lasted from December 2009 to February 2011.