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SSTGFLS J222557+601148 is a planetary nebula in the constellation Cepheus. Located between 2000 and 3000 parsecs distant from Earth, it was originally classified in 2006 as a supernova remnant. Thought to be the first supernova remnant first detected in the infrared wavelengths, the spectrum and properties of the object did not match up well with that of a typical supernova remnant, and it was reclassified as a planetary nebula in 2010. A candidate central star has been identified, with an apparent infrared magnitude of 22.4.

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  • SSTGFLS J222557+601148 (in)
  • SSTGFLS J222557+601148 (en)
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  • SSTGFLS J222557+601148 adalah sebuah nebula planeter di rasi Cepheus. Nebula ini terletak antara 2000 dan 3000 parsek dari Bumi. Pada tahun 2006, objek ini diklasifikasikan sebagai sisa supernova. Dianggap sebagai sisa supernova pertama yang terdeteksi pertama kali dalam panjang gelombang inframerah, tapi kemudian ditemukan bahwa spektrum dan sifatnya tidak cocok dengan sisa supernova pada umumnya. Objek ini kemudian diklasifikasikan ulang sebagai nebula planeter pada tahun 2010. Kandidat bintang pusat dari nebula ini telah diidentifikasi, dengan magnitudo semu sebesar 22,4. (in)
  • SSTGFLS J222557+601148 is a planetary nebula in the constellation Cepheus. Located between 2000 and 3000 parsecs distant from Earth, it was originally classified in 2006 as a supernova remnant. Thought to be the first supernova remnant first detected in the infrared wavelengths, the spectrum and properties of the object did not match up well with that of a typical supernova remnant, and it was reclassified as a planetary nebula in 2010. A candidate central star has been identified, with an apparent infrared magnitude of 22.4. (en)
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  • SSTGFLS J222557+601148 (en)
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  • EQ J222557+601158 (en)
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  • Originally misclassified as a supernova remnant (en)
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  • PLANETARY (en)
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  • SSTGFLS J222557+601148 adalah sebuah nebula planeter di rasi Cepheus. Nebula ini terletak antara 2000 dan 3000 parsek dari Bumi. Pada tahun 2006, objek ini diklasifikasikan sebagai sisa supernova. Dianggap sebagai sisa supernova pertama yang terdeteksi pertama kali dalam panjang gelombang inframerah, tapi kemudian ditemukan bahwa spektrum dan sifatnya tidak cocok dengan sisa supernova pada umumnya. Objek ini kemudian diklasifikasikan ulang sebagai nebula planeter pada tahun 2010. Kandidat bintang pusat dari nebula ini telah diidentifikasi, dengan magnitudo semu sebesar 22,4. (in)
  • SSTGFLS J222557+601148 is a planetary nebula in the constellation Cepheus. Located between 2000 and 3000 parsecs distant from Earth, it was originally classified in 2006 as a supernova remnant. Thought to be the first supernova remnant first detected in the infrared wavelengths, the spectrum and properties of the object did not match up well with that of a typical supernova remnant, and it was reclassified as a planetary nebula in 2010. A candidate central star has been identified, with an apparent infrared magnitude of 22.4. (en)
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