Stellarium / stellarium

Stellarium is a free GPL software which renders realistic skies in real time with OpenGL. It is available for Linux/Unix, Windows and macOS. With Stellarium, you really see what you can see with your eyes, binoculars or a small telescope.
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Mystery star near M51 #1192

Open LouisStrous opened 4 years ago

LouisStrous commented 4 years ago

Expected Behaviour

Don't show a magnitude-6 star near M51 where none exists in a picture I took recently.

Actual Behaviour

Stellarium shows an unnamed magnitude-6 star near M51 where none exists in a picture of the sky I took recently in an attempt to record M51, and where the Hipparcos catalog (via VizieR) doesn't list any stars within 15 arcmin. The unnamed star shows up already with only the default star catalogs installed (i.e., Configuration / Extras says "Get catalog 5 of 9").

My picture: mystery-star-picture

My picture shows stars down to about magnitude 10, so a magnitude-6 star should be very obvious. The three stars HIP 66116 - HIP 65768 - HIP 66004 near the location of the mystery star have magnitudes near 7 and are clearly visible, yet the mystery star is not to be seen.

Screenshot of Stellarium showing roughly the same FOV and showing the star's properties: mystery-star-stellarium

Note in particular that the star is listed by Stellarium to have a noticeable proper motion. If the star was really some part of M51 mislabeled as a star then you'd expect it to have no proper motion, M51 being way too far away to show a noticeable proper motion.

Steps to reproduce

In Stellarium, go to coordinates indicated in screenshot. Observe star.

System

github-actions[bot] commented 4 years ago

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ultrapre commented 3 years ago

@alex-w I decoded the stars/default/*.cat, found a fake star (fake hip id = 1316384 ) that extactly matches the one. The guide book notes that stars_1 and stars_2 give hipparcos catalogue, however some data of them has nonexistent hip num.

The same problem also exists in higher star data, the most serious is the actually nonexistent stars at the same position of bright Galactic Nuclei or globular cluster. For example, give a ramdom galaxy like NGC569, you can see a 13mag star in the center.

I advise to compile a new data from more accurate database like DR2, just compile a new cat data without changing code or both changing the star catalog format and code is okay. Picking the nonexistent stars one by one is difficult.

refer: https://wakata.nascom.nasa.gov//dist/generalProducts/attitude/ATT_SKYMAP.html http://www.rssd.esa.int/index.php?project=HIPPARCOS http://cdsarc.u-strasbg.fr/viz-bin/Cat?I/239 http://www.astro.ku.dk/~erik/Tycho-2/ http://www-gsss.stsci.edu/Catalogs/Catalogs.htm http://www-gsss.stsci.edu/Catalogs/GSC/GSC1/GSC1.htm http://www-gsss.stsci.edu/Catalogs/GSC/GSC2/GSC2.htm http://www.sai.msu.su/groups/cluster/gcvs/gcvs/ http://ad.usno.navy.mil/wds/ http://ad.usno.navy.mil/wds/orb6.html http://nstars.nau.edu/nau_nstars/ http://www.recons.org/ ……

gzotti commented 3 years ago

You advise "just" using DR2. Great. How do we deal with the few hundred missing stars from DR2? I mean those on the bright end... And no, the format should change and take 3D motion into account. Just that "someone" has to find enough time do it.