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Archive 1Archive 2

Modern legacy trivia

In my personal opinion this section is becoming a haven for complete trivia. Any suggestions on how we can include what is significant and exclude the marginal stuff (other than with a mechanical back-hoe)? Perhaps all other uses of the name Sirius should be moved to the disambiguation page? Thanks.—RJH (talk) 21:25, 13 October 2008 (UTC)

Well I decided to be bold and haul it off.—RJH (talk) 21:34, 13 October 2008 (UTC)
Common sense and some worldliness are good at sorting wheat from chaff. Not sure about Stockhausen (and waiting for sources above I see) but other material (eg boats/engines etc.) is pretty stock-standard. Its status as #1 star so to speak is pretty prominent and clearly the reason for its widespread use. As long as the article is kept an eye on it will be fine. I loath reductionis splitting of articles. Interpreation began in prehistory and continues to 2008. Cheers, Casliber (talk · contribs) 22:30, 13 October 2008 (UTC)
No Stockhausen reference has been forthcoming, so I was bold and removed the questionable text.—RJH (talk) 22:29, 17 December 2008 (UTC)

Possibility of planets

It would be nice to have a section about planets, as we do in the article of Alpha Centauri. What do we currently know about it? —Preceding unsigned comment added by 90.195.11.7 (talk) 14:38, 8 November 2008 (UTC)

The "Discovery of a companion" section covers the topic of another companion.—RJH (talk) 01:30, 10 November 2008 (UTC)
It would be nice if you could add some measure of distinction between stars and planets unless you are trying to be intentionally obstructive.

Red Sirius

Gee, I published two lengthy papers in the Journal for the History of Astronomy (1992 or 93) and a doctoral dissertation about the ancient Greek and Latin texts and the ancient folkore regarding Sirius with a focus on the red question, and I don't even get a footnote? What about Jay Holmberg's recent book on Sirius?

This poorly researched article really gives me pause about trusting Wikipedia....

Roger CeragioliRceragioli (talk) 06:12, 13 November 2008 (UTC)

What do you mean what about Jay Homberg's book? I read it preparing this article and it is refrenced quite a bit... Cheers, Casliber (talk · contribs) 08:34, 13 November 2008 (UTC)
Thank you for mentioning your research. As Casliber mentioned, Sirius: Brightest Diamond in the Night Sky, is included among the references. It looks like this is one of the papers you mentioned:
Ceragioli, R. C. (1995). "The Debate Concerning 'Red' Sirius". Journal for the History of Astronomy. 26 (3): 187–226. Retrieved 2008-12-11.
I couldn't find the others online, but that article certainly looks in depth.—RJH (talk) 18:14, 10 December 2008 (UTC)
I looked through the paper and concluded that there is more material than can possibly be incorporated in this article without running into WP:LENGTH concerns. It should really be the topic of a separate article, but I did include it as a reference for one of the sentences. It can be used by an interested reader to corroborate the multiple Homberg references.—RJH (talk) 22:27, 17 December 2008 (UTC)

"first noted by amateur astronomer Thomas Barker ... 1760" I seem to recall it's in Micromégas by Voltaire, 1752. Admittedly that's a work of fiction by an author not greatly noted as an astronomer. 198.142.41.56 (talk) 03:14, 3 January 2009 (UTC)

I want to add the newer idea for the "Sirius red" discussion, that the person

seeing Sirius as RED is interacting with Sirius , a special human trait... and yep its a long way (50 trillion miles ?) , but that that IS what occurs; and so if you see Sirius as RED (or moving away or fleeing), you are a special human indeed and can "connect" in that manner (ahead of the coming poo's poo's, if you experience this you will "understand)... /s/ lil red Jay 69.121.221.97 (talk) 14:28, 20 June 2009 (UTC)

Does anybody has a reference for an explanation based on color blindness of the observers? Keep in mind that most of the observers quoted were men and men have a 7 to 10% incidence of red-green color blindness, why would Seneca or Ptolemy be trusted when they said it was red? There's a pretty high probability that they were color blind. man with one red shoe 02:23, 3 July 2010 (UTC)

By the way, from Blue: "Ancient Greek lacked a word for blue and Homer called the colour of the sea "wine dark", except that the word kyanos (cyan) was used for dark blue enamel." -- that might explain Ptolemy description. man with one red shoe 02:41, 3 July 2010 (UTC)
Which of course could be a crap theory put in Wikipedia, because Homer might have simply poetically described a sunset at sea... man with one red shoe 02:50, 3 July 2010 (UTC)
Maybe not so much colour blindness as a colour bias such as deuteranomaly -- see here [1]. Skeptic2 (talk) 00:55, 13 August 2010 (UTC)
About deuteranomaly "This is the most common form of color blindness". Interesting that some people reported it red on this talk page, and the explanation seems to be the atmospheric conditions. So it might be a mix bag of explanations. In any case we are speculating here, we need references. man with one red shoe 02:25, 13 August 2010 (UTC)

red connection

Such red connections fall into the newer ideas concerning "entrainment" , entrainment comms and those are understood to have NO distance limitations at all; but also while not simultaneious, are nearly so; ab ? 15 secs 50T miles out, 50T miles back to acquire and "see red". box car willie, /s/ red eye wedjet 69.121.221.97 (talk) 14:41, 20 June 2009 (UTC)

Sirius Heliacal Rising

This is mentioned in the article but there should be added a ongoing date for the rising as presently it is to be in 2009 ???? about first of August ? ; ... and perhaps this year, 2009, the more important date is the date of the rising of ORION, ? 1 month earlier, which coincides with important events clearly prophecied in Egyptian rite diagrams from 3-6,000 years ago , i.e. the arrival of Horus .../s/ showshenk 129th, sphinx face willy 69.121.221.97 (talk) 14:34, 20 June 2009 (UTC)

Assuming I comprehend what you are attempting to communicate, I have to disagree. Wikipedia is not an ephemeris.—RJH (talk) 16:38, 23 June 2009 (UTC)

Galaxy?

I'm obviously not well versed in astronomy, so this question might seem naïve to the initiated, but why doesn't the article mention the galaxy to which this star belongs? I assume it's the Milky Way, but, again, as a lay person, that would need to be stated explicitly for me to know it. __meco (talk) 10:03, 10 December 2008 (UTC)

Hello Meco. Yes it's in the Milky Way, as are virtually all named stars. I guess, because of the distance, it's just seems like one of those semi-obvious things, like saying you live in a city that's on planet Earth. But it may make sense to add some information about the orbital parameters of Sirius through the galaxy.—RJH (talk) 17:56, 10 December 2008 (UTC)
Well, I was hoping that there would somehow be a mention of this fact. As I stated, this is not so obvious to everyone. __meco (talk) 08:57, 11 December 2008 (UTC)
This fact would need to go on virtually every star article on wikipedia. I'm not sure of a gracious approach to this that would not be painfully obvious to many readers. (I.e. it would tend to get deleted.) Does anybody have a good suggestion?—RJH (talk) 15:37, 11 December 2008 (UTC)
Don't they all have the same infobox? At least it could go in the infobox as a semi-standardized item? __meco (talk) 16:23, 11 December 2008 (UTC)
Yes, I was thinking about that. It needs to be discussed at WP:ASTRO.—RJH (talk) 17:52, 11 December 2008 (UTC)
Is there actually a case where a star would not be in the Milky way (in regards to ones we have catalogued in any fashion)? Perhaps instead of adding "galaxy" to the infobox we can state which Milky Way arm the star belongs to, and have the "Arm:" part in the infobox redirect to Milky Way's section on the different arms. SkarmCA (talk) 16:58, 21 December 2008 (UTC)
Yes, most supernovae are observed in other galaxies. However, those articles have their own specialized template. I've read some news stories of referencing specific stars for use in measuring extra-galactic distances, such as here. I'm sure there are other examples. As for listing the region of the galaxy, I think that would make an interesting addition if a source could be found. Another possible addition is to list its stellar association, such as a moving group. If we did that, then it could default to Milky Way.—RJH (talk) 17:23, 22 December 2008 (UTC)

Metalicity?

In the Sirius Supercluster section, it says "the Ursa Major Group has an estimated age of 500±100 million years, while Sirius, with metallicity similar to the Sun's, has an age that is only half this, making it too young to belong to the group". The middle bit: "with metallicity similar to the Sun's" is suspect. It seems to contradict material elsewhere in the article. Also a star with metallicity similar to the Sun's would likely have similar age to the sun, ie much older than this. Would someone who understands this better than me please check the references? 198.142.41.56 (talk) 03:35, 3 January 2009 (UTC)

Per the Liebert et al (2005) reference, "most stars in the solar neighborhood have close to solar abundances". Sirius' outer atmosphere is enriched with metals, giving the high surface metallicity. But this doesn't tell us what the interior composition is like; I think it's just assumed to be solar based on a comparison with other similar stars of known ages. (For example, the Hyades cluster as in Liebert.)—RJH (talk) 20:28, 5 January 2009 (UTC)

the sentence struck me as completely nonsensical as well. inference's about the stars invisible interior besides i think it should be at least logically explained. i take it there is a reason better then this to assume it is not part of that certain group. btw i propose the two main stars merged into a binairy system later on, because i see no reason the (now) beta sirius would turn into a red giant when the rather similar alpha didn't. (or is at least not described to show signs of such a progressed evolution). mh next i wonder if the evasive third companion may have played a role in metallicity , and perhaps even formed a base for the ancient writers description of the star as red, since it is my impression those tried to incorporate knowledge that was ancient already then.. in that sense a chinese name like 'the white star' somehow suggests it was important to mention it's colour , perhaps as in, "the definitily not anymore red star..". just my take , but please change that sentence into something that makes sense.24.132.171.225 (talk) 07:18, 7 February 2010 (UTC) reading on in the comments i see there is some sirius mystery going about, but my comment refers just to this wikipedia article, i have no idea what this mystery is about nor was i aware of some such controverse when i commented.24.132.171.225 (talk) 07:26, 7 February 2010 (UTC)

Anything is possible, but a merger seems very unlikely unless it was a merger of two binary systems. The reason the white dwarf already passed through the red giant stage is that it started off with more mass. I thought this was quite clearly explained in the article. The Sirius A section also explains the metallicity issue, so it is not inconsistent. I invoke Occam's Razor for the remainder of your comments.—RJH (talk) 16:58, 7 February 2010 (UTC)

Lead sentence

Since this article is about the binary star system (and not just Sirius A) shouldn't the first sentence be something to the effect of "Sirius is a binary star system perceived as the brightest star..."? Strikehold (talk) 09:09, 2 April 2009 (UTC)

This is the sort of major headache we get with all bright binaries..... :( ummm, technically I sort of agree, but given the size it is like what is seen is the star (essentially Sirius A) and its little faint (but heavy companion). I will wait and see what others think. Casliber (talk · contribs) 11:40, 2 April 2009 (UTC)
True what is perceived is Sirius A, but the article itself is about the binary system, not just Sirius A. I think the lead paragraph is somewhat self contradicting, starting: "Sirius is the brightest star in the night sky...", but then concludes "...What the naked eye perceives as a single star is actually... Sirius A and... Sirius B." (i.e. "Sirius" cannot be both the brightest star and two distinct stars).
Since the first sentence in a paragraph should sum up the paragraph, and the first paragraph should sum up the article, I think the most appropriate first statement would say that "Sirius is a binary star system consisting of white main sequence star Sirius A, which appears as the brightest star in the night sky, and white dwarf companion star Sirius B"... Or something to that effect. Strikehold (talk) 12:21, 2 April 2009 (UTC)
Professor Kaler's description takes a similar approach to the summary on this page.[2] The current description focuses on what is relevant to most readers; the apparent brightness of the star. Thus I think it's fine just the way it is now.—RJH (talk) 19:42, 2 April 2009 (UTC)

Sirius C

It has been stated as a binary star, but there is evidence of a third star that has been named as Sirius C, which also follows the elliptical orbit just like Sirius B does. citation [3] —Preceding unsigned comment added by 122.167.2.39 (talk) 20:20, 20 June 2009 (UTC)

Not a reliable source, sorry. I have seen some pretty exhaustive discussion on the subject. Casliber (talk · contribs) 21:12, 20 June 2009 (UTC)
batting 1,000 - the more important aspect of Sirius and its neighboring star is they rep the Dog constellation, but even more accurate is they are the "bat" which activates to Pull upwards the soul of the aspirant, see Lord Pacal booklet imbedded in his tombstone cover ... so Mayan, Egyptian understandings merge in their diagrams to indicate a global understanding of Sirius as Isis , bat, etc joe the bat battaglia 69.121.221.97 (talk) 01:09, 2 July 2009 (UTC)
Just don't go out at night and you'll be okay.—RJH (talk) 15:27, 2 July 2009 (UTC)

assuming it exists (the paper, not the star, i can't access aanda.org to search at the moment, a glitch in the matrix?) who can comment on this article? Daniel Benest and J. L. Duvent, “Is Sirius a Triple Star?”, Astronomy and Astrophysics, vol 299, 1995, pp. 621-628.204.210.134.40 (talk) 03:43, 3 August 2009 (UTC) OK I found it in, of all places, the sources for this article. i'm not an astrophysicist, and i slept thru Fourier analysis in school, but it looks like it's been detected but not observed, like B in 1844? 204.210.134.40 (talk) 04:19, 3 August 2009 (UTC)

The Benest & Duvent article merely suggest that a third body exists. But, after all, it is based on data with some noise, and humans are good at finding patterns where none exist. You might want to take a look at the Kuchner & Brown (2000) paper cited in this article, which involved an infrared search for a companion.—RJH (talk) 18:57, 3 August 2009 (UTC)
Someone tried to push the 'third companion' business in this article earlier this year, no doubt with the Sirius Mystery nonsense in mind, but the Bonnet-Bidaud and Pantin paper referenced in the article is pretty definitive. Odd how these 'third star' believers always reference the older papers where the answers are not quite conclusive rather than the more recent stuff, isn't it? Skeptic2 (talk) 19:31, 3 August 2009 (UTC)

The discovery of the proper motion of Sirius

The current text claims that Halley discovered the proper motion of Sirius by comparing his St Helena observations with those of Ptolemy (precessed to Halley's epoch). However, Halley's original paper in the Philosophical Transactions (vol. 30 [1717/19], pp. 736-738) does not refer to any measurements made from St Helena. Nor is Sirius listed in Halley's 1679 southern star catalogue. In fact, Sirius is used several times in this catalogue as a reference star (with assumed coordinates, taken from Tycho Brahe's star catalogue) for determining the positions of stars in its vicinity. Although Halley does not give any details for the modern measurements he used, it is far more likely that he compared Ptolemy's stellar positions with those made by John Flamsteed at Greenwich. I suggest to modify the current text to reflect this. (AstroLynx (talk) 16:10, 26 June 2009 (UTC))

I think you're right. The Holberg source doesn't actually say Halley compared his own observations against those of Ptolemy; only that he compared contemporary star positions against those of Ptolemy.—RJH (talk) 18:46, 26 June 2009 (UTC)
Sadly I returned the Holberg book to the library, but I trust RJH to do the right thing - :) Casliber (talk · contribs) 19:45, 26 June 2009 (UTC)
Actually Holberg 2007, p. 41 can be previewed on Google.—RJH (talk) 16:42, 28 June 2009 (UTC)
Interesting. The two pieces of information are juxtaposed in the text which (I think) I took as meaning he used his own. However, it does not say that he used his own. In any case, have a go at it Astrolynx. Now if only someone wrote a book like this on Canopus...Casliber (talk · contribs) 21:05, 28 June 2009 (UTC)

Questions for lovers of Sirius

Is there any interest in creating a bibliography of recommended books and authoritative, scholarly sources on this topic? Personally I also want to know about fictional and other non-scholarly accounts of Sirius; that it is stuff that is hardest to pin down. Neredowell (talk) 02:31, 4 January 2010 (UTC)

In general, I find bibliographies of little use. If something is integral to the understanding of the article, it will have been used as a source, and hence will be somewhere in the reference list. For this article, this book:
  • Holberg, J.B. (2007), Sirius: Brightest Diamond in the Night Sky, Chichester, UK: Praxis Publishing, ISBN 0-387-48941-X
was a fascinating read and will have a host of notes in the back on what else to read. cheers, Casliber (talk · contribs) 03:13, 4 January 2010 (UTC)
The fictional accounts are covered by the "Sirius in fiction" article. Something like a list of "recommended books" would be difficult to build and maintain because it is very much a matter of personal judgment rather than something we can cite. Everybody is going to have a different opinion on what is a quality addition, so it could become a dumping ground for every possible work on the subject. I think it's better to avoid that type of situation.—RJH (talk) 16:08, 4 January 2010 (UTC)
Yeah, and it'll end in tears when it will be (inevitably) pruned....Casliber (talk · contribs) 19:28, 4 January 2010 (UTC)

Needs a citation

The following entry has been tagged since January as needing a source, so I'm moving it here until it can be addressed.

It is the subject of more myth and folklore than any other star apart from the sun.[citation needed]

Since it is a broad opinion, I'm not sure a suitable source will be available.—RJH (talk) 16:56, 5 July 2009 (UTC)

Something etlls me it might be from the prologue of the Holberg book (???) My connection is slow and my plate is full...RJH can you check that? Sorry, Casliber (talk · contribs) 01:47, 6 July 2009 (UTC)

Using siriusascension.com as a source

This site is registered to Paul McCarthy of Brighton and appears to exist to promote his commercial activities as a "spiritualist". The site should not be used as a source as it fails WP:SPS and WP:SPAM.—Ash (talk) 06:15, 15 September 2009 (UTC)

Thanks for investigating the dubious source.—RJH (talk) 22:22, 15 September 2009 (UTC)

This article is impossible!

This article is next to impossible to edit! Where most articles are mostly text with little wikimarkup, this article is the inverse.

For example, the references are all listed in the expanded form like this:


<ref>{{cite web
| last=Ridpath | first=Ian | year=1978 | url=http://www.csicop.org/si/7809/sirius.html|title=Investigating the Sirius "Mystery"
| publisher=Committee for Skeptical Inquiry
| accessdate=2007-06-26 }}</ref> More recently, the contaminators have been suggested to be the [[ethnographers]] themselves.
<ref>{{cite web
| url=http://www.ramtops.co.uk/dogon.html
| title=The Dogon Revisited
| accessdate=2007-10-13 | first=Bernard R. Ortiz
| last=de Montellano }}
</ref><ref>{{cite web
| url=http://www.philipcoppens.com/dogonshame.html
| title=Dogon Shame | accessdate=2007-10-13
| first=Philip | last=Coppens }}</ref> Others see this explanation as being too simplistic.<ref>{{cite journal
| last=Apter | first=Andrew
| title=Griaule’s Legacy: Rethinking “la parole claire” in Dogon Studies
| journal=Cahiers d’Études africaines
| year=1999 | volume=45 | issue=1
| pages=95–129 | url=http://www.sscnet.ucla.edu/history/apter/Cahiers.pdf | accessdate=2008-04-16 | format=PDF }}</ref> In his book ''Sirius Matters'' Noah Brosch proposed that the astronomical cultural transfer to the Dogon took place in 1893, when a French eclipse expedition visited their region.<ref>

This makes the article a nightmare to work with. -RadicalOne•Contact Me•Chase My Tail 17:14, 7 February 2010 (UTC)

I have to politely but completely disagree. The expanded citations are much cleaner and easier to work with.—RJH (talk)
The citations are easier, sure. What about the actual article? -RadicalOne•Contact Me•Chase My Tail 19:10, 7 February 2010 (UTC)
Wasn't my idea to expand the refs out, but it is workable. Just cntrl-F the piece of text you're looking for to edit. I've found this the easiest way after fumbling about in a segment of prose heavy with refs. cheers, Casliber (talk · contribs) 19:40, 7 February 2010 (UTC)
I tried that. There are so many references (a good thing) that they make it impossible to find the prose without having to search for each sentence individually. -RadicalOne•Contact Me•Chase My Tail 19:50, 7 February 2010 (UTC)

A solution would be to modify the article to use WP:LDR. That makes it much easier to find the prose.—RJH (talk) 15:07, 4 July 2010 (UTC)

Sigh. If someone wants to do that I wouldn't mind. I hadn't thought about it too much till now but some other editors are doing it and I might start from now on. Casliber (talk · contribs) 15:11, 4 July 2010 (UTC)
Well, in the future there might be a tool to do it for an entire article. (Or at least I can hope so.) At present I usually just use it when I add new citations.—RJH (talk) 15:46, 4 July 2010 (UTC)

Agreed that it was impossible - I've modified all the references to use WP:LDR, much easier to find your way around the text now! Hopefully I haven't broken anything while doing so. Couple of points I noticed, firstly that the references I have assigned the names Jiang1992 and Jiang1993 look like they may be the same thing (author is the same and the horribly mangled autotranslation of the title I used looks like it could plausibly be the same), even if not the Jiang1992 reference could perhaps be updated so you don't have to understand Chinese characters to be able to read it. Secondly the book Brosch (2008) is cited both as a normal reference and in the "cited texts" section, not sure if that is an issue or not. Icalanise (talk) 21:02, 21 July 2010 (UTC)

According to CNKI, Jiang1992 is in Acta Astronomica Sinica (天文学报), 1992, #4. [4][5] Spacepotato (talk) 21:58, 21 July 2010 (UTC)

Colour of Sirius

To me, Sirius is neither red nor bluish white but yellow.--80.141.181.193 (talk) 23:52, 12 March 2010 (UTC)

I'd love to see more information about the odd appearance of this star - outside of quack theories about red giants and mistranslations, that is. I was surprised to find that from central Pennsylvania last winter this star was so dramatically red-flashing it was like a police siren in the sky - thinking it was a star was the fourth hypothesis that came to mind. Looking for discussion of this, I found similar comments from Dublin [6] and many other forums; it's tremendously striking even to people ordinarily uninterested in astronomy. And apparently this is visible telescopically, and not just an effect in the eye.
It would be splendid if some Wikihero out there can generate video from an amateur telescope documenting the effect... Wnt (talk) 10:55, 12 August 2010 (UTC)
The answer seems to be atmospheric disturbance - I have not seen it discussed in astronomy book that I can recall..? I have never seen it do this but I am in Sydney so it is always way up high when I notice it....:) Casliber (talk · contribs) 11:20, 12 August 2010 (UTC)
Yes, it's atmospheric scintillation – or 'twinkling' in plain English. One reason why Sirius is reported as a multicoloured UFO from time to time. Skeptic2 (talk) 00:49, 13 August 2010 (UTC)
That's what everyone says. But why does this one star twinkle in such a special way? Is it strictly a matter of magnitude, that the red is invisible for other stars; or could the angular diameter somehow affect what we see from the diffraction? Wnt (talk) 06:42, 13 August 2010 (UTC)

incorrect data

The side box lists Sirius B has having luminosity .026, which is 1000 times less than Sirius A's luminosity of 26. In the text of the article, though, is "Currently 10,000 times less luminous in the visual spectrum, Sirius B was" both are referenced. someone needs to check the references and resolve the discrepancy. I am pretty sure Sirius B has luminosity of .0026. -- 192.203.222.68 (talk) 16:23, 6 April 2010 (UTC)

The total luminosity should be greater than the luminosity in the visual spectrum.—RJH (talk) 16:28, 6 April 2010 (UTC)

Heliacal rising

I don't quite grok this sentence: "Egyptians based their calendar on the heliacal rising of Sirius, namely the day it becomes visible just before sunrise after moving far enough away from the glare of the sun." Does it mean that the star is actually above the horizon for a few days, but we can't see it because of the glare of the sun? Noloop (talk) 01:23, 2 July 2010 (UTC)

Yes. The zodiac works the same way. There are times when a star is only above the horizon in the daytime, and hence invisible due to the sun's glare, and this gradually changes over the course of the year so a star is visible during the night. Casliber (talk · contribs) 01:37, 2 July 2010 (UTC)
The Moon, which may be more familiar, does the same thing in reverse, since it travels faster around the sky. At new moon, it isn't visible (barring an eclipse), but a couple of days later it's trailing the sun by a large enough angle to show a thin crescent, which sets shortly after sunset.
—WWoods (talk) 07:48, 2 July 2010 (UTC)

"Bold text"?

  • At the very top of the article, it says "Bold text". When I try to edit the article to remove it, I don't see that phrase anywhere. I'm not sure what happened, but can someone fix it? Erpert (let's talk about it) 19:29, 2 July 2010 (UTC)
    • It may have been an experimental edit by somebody. The entry was likely reverted by the time you went to edit it. Rubbish like that tends to happen to front page articles. I wouldn't worry; the article will get cleaned up.—RJH (talk) 20:44, 2 July 2010 (UTC)
      • I checked it today and it seems in pretty good shape. Just a couple of minor things need addressing.—RJH (talk)
        • It's possible to find such things from the History tab - using the date of your post, I quickly found [7] and [8] (one minute apart). Probably someone completely unfamiliar with Wikipedia made the first one. Wnt (talk) 15:25, 13 August 2010 (UTC)

Merge from Gliese 244 B

The following discussion is closed. Please do not modify it. Subsequent comments should be made in a new section. A summary of the conclusions reached follows.
Looks like a good consensus to merge. Done -- Icalanise (talk) 00:51, 4 July 2010 (UTC)

I suggest merging the article Gliese 244 B into this one and have Gliese 244 B turned into a redirect: the material there is already adequately covered here. Icalanise (talk) 12:12, 3 July 2010 (UTC)

  • Support—Gliese 244 B is just a weak clone of what is already mentioned on this page. The Sirius B section should be better developed before forking off a child article.—RJH (talk) 16:20, 3 July 2010 (UTC)
  • Reluctantly Support My gut feeling is absolutely to oppose such mergers in order to encourage development of the subtopic. But I cannot for the life of me see creating a separate article for the system as opposed to Sirius A. So, while it pains me to say it, logically, Sirius B needs to become a redirect.μηδείς (talk) 22:02, 3 July 2010 (UTC)

Sirius A and B images

All the images in this article show the companion star, Sirius B, positioned apparently close to the main star, Sirius A, including in the Hubble image. Depending on the relation of our point of view to the system's orbital plane, this may be a fairly common observation when viewed from Earth. However, the distance seperating the two bodies is listed here as range between 8.1 and 31.5 AU. These distances are vastly greater than the proximity the images would suggest.

My concern is that the reader may get the impression the two stars are positioned very close to each other as depicted in the images. Some may also assume this apparent close proximity is the only reason the two appear as a single star with the naked eye (in other words they would both be visible if there were greater separation), when this may not necessarily be the case, and when in fact the separation is significantly greater than it appears in these images. For the two to be visible with the naked eye, the separation may have to be far greater than 31.5 AU. I don't know. But I'm wondering if we should add something somewhere in the article to clarify that the two are actually not nearly as close as they are depicted in the images.Racerx11 (talk) 14:38, 27 November 2010 (UTC)

Yes, I think that would make sense. We would probably need to add a note computing the ratio of the separation to diameter of Sirius A. At the minimum of 8.1 AU, that should be about ×1018.—RJH (talk) 18:29, 28 November 2010 (UTC)

Orbital parameters

I have made some edits to the orbital parameter info table at the top. First, I have reverted a spurious edit from 2009-10-13 where the orbital period has been changed from 50.09 years to 49.9 years without reference (also in the text). Then, I have replaced the citation of Gatewood & Gatewood 1978 by citing van den Bos 1960, the original reference, Gatewood and Gatewood are citing themselves. Maybe the data should be updated by a more recent parameter set by Benest & Duvent (1995), but van den Bos seems to be some kind of standard so far. Benest & Duvent also do not provide uncertainties to their fit. It is yet unclear to me, why Gatewood & Gatewood use a semi-major axis of 7".56 while van den Bos find 7".50. Maybe some mistype or whatever. 7.50 is nevertheless closer to the value from Benest & Duvent of 7.501.

Anyway, I will have to update the orbit figure of Sirius B since it is still based on the obviously wrong period of 49.9 years (which I didn't know at that moment).--SiriusB (talk) 14:28, 9 August 2011 (UTC)

Yes, the present data matches the values listed in the USNO's Sixth Catalog of Orbits of Visual Binary Stars (2006), so that's probably fine. Thanks. Regards, RJH (talk) 14:52, 9 August 2011 (UTC)
The 49.94 year figure comes from Volet (1929), but it is still widely quoted in books, and apparently by others who should know better. van den Bos (1960) gives the 50.09 year orbit. Conveniently, the Sirius orbit has just been studied including modern observations and published in Bond et al (2017). I have updated the article accordingly. Quite possibly, values will continue to be reset by people who "know better" - c'est la vie. Lithopsian (talk) 13:37, 20 August 2017 (UTC)

Detection of weak magnetic field on Sirius

Petit, P.; et al. (2011), "Detection of a weak surface magnetic field on Sirius A: are all tepid stars magnetic?", Astronomy & Astrophysics, 532, Bibcode:2011A&A...532L..13P, doi:10.1051/0004-6361/201117573 {{citation}}: Unknown parameter |month= ignored (help)

Regards, RJH (talk) 22:21, 7 October 2011 (UTC)

Closest stat that can be seen with the naked eye?

This claim is not true, one can see the Alpha Centauri binary star system with the naked eye and it roughly half the distance to earth as Sirius. — Preceding unsigned comment added by 112.160.102.179 (talk) 12:13, 17 May 2012 (UTC)

The article qualifies the claim by limiting it to observers north of 30 degrees latitude. Alpha Centauri is never visible for much of the Northern Hemisphere.--Trystan (talk) 13:19, 17 May 2012 (UTC)

Too unclear

I do not see the point in having an article like this in Wikipedia. This project supposes to make things easier to common people. This article seems to be written for astronomers only. I really miss Carl Sagan and his campaign to make astronomy near to the people. The authors of this article are just hedonist guys copying hermetic books from their lazy library. Regards, Prof. McClain. — Preceding unsigned comment added by 175.100.93.5 (talk) 02:56, 18 June 2012 (UTC)

Well it's unfortunate that you feel that way. I can see by your IP address that you're writing this from Phnom Penh in Cambodia. I didn't know you folks followed Carl Sagan. Regards, RJH (talk) 16:19, 18 June 2012 (UTC)
On the contrary, I find this article has just the right amount of unclarity. μηδείς (talk) 18:38, 18 June 2012 (UTC)
Errrr, Medeis, you've lost me....... Casliber (talk · contribs) 20:31, 18 June 2012 (UTC)
The section header suggests the article is "too unclear". I disagree. It has just the right amount of unclarity. μηδείς (talk) 20:42, 18 June 2012 (UTC)
Frankly, I am not an astrologer, and even I had no problem making out the article. As for funny headers, my local library has a sign posted "Please do not overstuff the toilets." It prompted me to ask the reference librarian just how stuffed they wanted the toilets μηδείς (talk) 20:45, 18 June 2012 (UTC).
Aaah right. Casliber (talk · contribs) 20:52, 18 June 2012 (UTC)
Looks like this is the anon.'s only contribution. It may simply be flame bait, rather than an attempt at meaningful dialogue. Regards, RJH (talk) 20:34, 19 June 2012 (UTC)
That's not nice. With comments like that I can understand that someone does not want to be identified. Note that dynamic IPs usually change often and if the person can't afford an internet connection then they are likely to use a variety of devices/locations. I am often frustrated by Wikipedia articles that seem to be written by people that want to show off. Sam Tomato (talk) 06:35, 11 March 2017 (UTC)

Blue shift

"Sir William Huggins examined the spectrum of this star and observed a noticeable red shift. He concluded that Sirius was receding from the Solar System at about 40 km/s. Compared to the modern value of −7.6 km/s..."

Assuming the "modern value" is correct, the star actually has a blue shift, and the statement that he observed a red shift is incorrect. Wouldn't it be more accurate to say "he thought he observed a red shift"? 184.99.28.92 (talk) 02:59, 2 September 2012 (UTC)

Sirius as it appears in the night sky.

So there's a giant star-cross filter somewhere between Sirius and the Earth? Paul Magnussen (talk) 16:25, 27 June 2013 (UTC)

Maybe the infobox image is not that useful then....Cas Liber (talk · contribs) 20:30, 27 June 2013 (UTC)
...or at least the caption isn't --RacerX11 Talk to meStalk me 21:54, 27 June 2013 (UTC)

I have removed the words "as it appears" from the caption. Not sure if that's what you had in mind, but it seemed to me a harmless fix for the moment. We could add a disclaimer like "The cross-patterned spikes radiating from the star are photographic artifacts", but I don't feel that's necessary at all. Of course anyone is still welcome to replace the image with something better. --RacerX11 Talk to meStalk me 12:43, 30 June 2013 (UTC)

I guess we have a few pictures of a bright star on a dark sky. Not sure if we need all of them. Cas Liber (talk · contribs) 13:42, 30 June 2013 (UTC)
You're right, we can remove it altogether. Most of our articles on stars just have a map for their infobox image. Do you think that's best? RacerX11 Talk to meStalk me 14:11, 30 June 2013 (UTC)
Yeah I think leave map image on its own Cas Liber (talk · contribs) 20:22, 30 June 2013 (UTC)

Wrong Hieroglyph

The hieroglyph shown at the start of "observational history" is a fake and should be removed. It is a crudely redrawn rendition of a drawing of three separate hieroglyphs that were originally in different rooms. It doesn’t take much searching to find that some historians individually and without much evidence ascribe to Sirius the Egyptian symbols of the pyramid, the dog, the cow and even the seven-petalled flower. It could even be that all of these are wrong, nobody really knows what the hieroglyph for Sirius was. Mollwollfumble (talk) 12:03, 30 June 2013 (UTC)

Hmmm, don't recall how that got in the article (whether I got it out of a book or someone else added it, I forget now). Need to re-check.....Cas Liber (talk · contribs) 13:43, 30 June 2013 (UTC)

The article states that Alvan Clark's 18.5" lens was made for Dearborn Observatory. It did end up at Dearborn, but the lens was made for the University of Mississippi. In fact, the glass for the lens was obtained in Europe by the University's chancellor, F. A. P. Barnard. The outbreak of the American Civil War prevented the lens from being delivered to the University of Mississppi, and it was obtained by Northwestern University. This is a widely known fact and should be corrected in the article. — Preceding unsigned comment added by 108.131.82.16 (talk) 02:38, 9 February 2014 (UTC)

First Sentence

The first sentence states "Sirius is the brightest star in the night sky." Shouldn't this say something more along the lines of "Sirius is the brightest star in the night sky as observed from Earth" or "Sirius is the brightest star in space that can be viewed from Earth?" If you agree, let me know and I can make the edit, thank you Triforces (talk) 17:37, 27 June 2014 (UTC)

No, because no-one can observe it from a significant distance outside the solar system so the rewording would be superfluous. — Preceding unsigned comment added by Historikeren (talk • contribs) 21:01, 28 July 2014 (UTC)

Shouldn't be there an article about Sirius B?

Consensus is to retain information on Sirius B at this article. DrKay (talk) 15:20, 22 February 2015 (UTC)

The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

It is a binary system, but Sirius B is a different star with different characteristics. It should have its own article Tetra quark (talk) 04:13, 17 December 2014 (UTC)

Maybe - it would only be worthwhile if someone was willing to make the article and intending to put more into it right now than the parent article. Otherwise it would be pointless reduplication of content. Cas Liber (talk · contribs) 05:33, 17 December 2014 (UTC)
@Casliber]: I wouldn't copy the information. I'd move it to the new article. I'm willing to create that new article Tetra quark (talk) 14:04, 17 December 2014 (UTC)
That would not be a good idea and I would revert it. The information in this article is (I see) at the right level of detail. It is a component of the Sirius system and hence needs to be a part of this article. If you were going to research and write quite a bit more from online sources then that would be great. There are loads of star redlink articles to write without disrupting established articles. Cas Liber (talk · contribs) 19:54, 17 December 2014 (UTC)
The thing is that the Sirius article is about the star, not exactly the system. Sirius B is another star. As you may know, I have created the new article but it redirects to the main one as of now. Here is a link that doesn't redirect you: https://en.wikipedia.org/w/index.php?title=Sirius_B&redirect=no .....I guess I can rewrite that. Tetra quark (talk) 20:15, 17 December 2014 (UTC)

I strongly oppose this. When we say "Sirius", it is about the entirety of the star system. (Capella has four components, yet it is only on one article). Many stellar systems are only in one article (Antares, Rigel, Algol, etc.), so I think Sirius B would remain as a section of the article Sirius. Problem here is if we created Sirius B article and get the full coverage of studies there, it would not gain notability because it is much less famous than Sirius A. To have the context, in the infobox of Sirius itself states "Sirius A/B". Plus, the white dwarf Sirius B is greatly tied with Sirius A. So I suggest to make it as a section on Sirius article. SkyFlubbler (talk) 21:05, 17 December 2014 (UTC)

Oppose; Personally, I don't think any star in a system should have its own article (that would include stuff such as vB 10, which I think should be merged). Since the system is inexorably tied together, it makes sense to discuss the system as a whole in an article, and not have separate articles for the components. StringTheory11 (t • c) 21:11, 17 December 2014 (UTC)
  • Oppose the proposal presented at WT:AST. We should not cut all the material about Sirius B out of the Sirius article. We should have a binary article somewhere, which should contain some information about both stars. If we split off Sirius B, then Sirius A should also be split off into a separate article, and another separate article should exist for the star system. The primary member of the system would like as not have a separate sub-article from the star system article before the secondary member. But the star system itself should be the primary landing point, and should any component have separate articles, then there should be a star system article around to deal with the entire system. -- 67.70.35.44 (talk) 05:45, 18 December 2014 (UTC)
  • Mega-Support Welcome to the odd world of astronomology, where we call Sirius "a star" because by unaided vision we cannot determine that there are two stars. Kind of like how we don't write articles about cell types in the brain, or other organs, since we can't visually distinguish neurons from glial cells in the cortex /irony. I have suggested before that we call it a system, this was shot down by the article's owners. What we probably need is an encyclopedia-wide RfC on whether systems with more than one star merit a small article on the system linking to larger articles on the separate stars (like we do with species in a genus) or whether we should keep one article, but reflect reality, and stop referring to Sirius as a star altogether, but call it a stellar system. In the meantime, at least we have a popular culture section. I support an RfC requesting a three way split, the system, and separate article on the stars. μηδείς (talk) 06:14, 18 December 2014 (UTC)
Thanks for the support. However, making three pages (sirius sytem, sirius A and sirius B) is not the idea I had in mind. When we say the word "Sirius", we are obviously referring to Sirius A, the brightest star in the night sky, not the system. The star was called Sirius long before Sirius B was even discovered. To sum it up, the main article should stay almost as it is. We just remove the section dedicated to Sirius B and paste it into the new article, which by the way I have already created (Sirius_B, however, I made this page redirect to the main article, so relax) Tetra quark (talk) 13:58, 18 December 2014 (UTC)
The thing is, we don't necessarily call it a star, we call it a star system, which it is. This isn't a scenario in which Sirius is simply an optical double star, in which case I would be all for having separate articles; rather, it is a true binary star system, where one cannot talk about one member without talking about the other as well. StringTheory11 (t • c) 04:19, 19 December 2014 (UTC)
  • Comment for the Russian (my keyboard does not type those text). It is not liable for W UMa variables, or stars which physically touch each other. Stars in systems have close relations; if we created articles about their components we may make duplicate articles.
For Sirius, it has been called a single star simply because antiquity says it's a single star, until the white dwarf was discovered. Now basically, "Sirius" refers to the two stars. If we created articles about their counterparts (say Sirius A, Sirius B, etc) then that would be duplication. Also, the stars are not that massive in detail to have their own articles, after all, stars are just balls of hot gases and nothing else. SkyFlubbler (talk) 09:48, 18 December 2014 (UTC)
  • Oppose removal of material (unless anyone is proposing to build a bigger article on Sirius B - but that would mean keeping the same content here and having more in a daughter article (in which case I would support the creation of that article) Cas Liber (talk · contribs) 13:50, 18 December 2014 (UTC)
  • Second Objection We must review first if people will view it. When you ask layman people about "Sirus B" they will just ask "What is it?!". My reason for this is because the article would be poorly viewed, unlike for the Sirius A. If we cut off all info on Sirius A and put it in B, surely people will never know what is B, because A is more famous and more viewed than B. SkyFlubbler (talk) 05:24, 19 December 2014 (UTC)
  • Strongly oppose: For consistency (and all the other oppose reasons above). Information from the CMa A article would need to be copied to CMa B. As time passes, and information changes/gets reworded/etc., the 2 pages would not move in lock-step and there would surely be page-drift. The star template has all relevant information on it, and a new user is able to accurately interpret the facts from a single page. The only reason another article should be made is if CMa B is ejected from the system in the future.   ~ Tom.Reding (talk ⋅contribs ⋅dgaf)  14:16, 19 December 2014 (UTC)
  • Support creating an article on Sirius B, not just a redirect. But retain content in this page. Extra detail can be added to the article on the B that is not put on this page. Splitting is how Wikipedia grows. It does not matter that so huge numbers of readers want to find it, as long as there are some. Drift does not matter either, as long as facts are consistent. Graeme Bartlett (talk) 07:22, 20 December 2014 (UTC)
  • Comment–If we did this on Sirius, we will ned to do it so for other stars as well. If we split Sirius B just because it has other characteristics from A, we must do that for other stars as well. Example is Antares A, a red supergiant and Antares B, a B-type main sequence. We must not split Sirius B because very few people will search for it, because very few people know about it. They know Sirius as "Dog Star, brightest star in the night sky" so splitting it would make confusion. We can split it if and only if it is only a visual companion, a coincidential alignment to our line of sight (i.e. Zeta Scorpii). If we did this for Sirius, other star articles must split also and that would cause a big problem for the entire WikiProject. Just because it has other characteristics does not necessarily mean it needs to have an article of its own. We must consider that we must deliver the data to readers as simple and as quickly as possible. If we split Sirius to A and B that would cause confusion. SkyFlubbler (talk) 13:41, 22 December 2014 (UTC)
  • Conditional support– Split the article if you can also split others. If only the split is that Sirius B is a different star, do that on others. But take note: of all the 9,500 stars visible by the naked eye, 3/4 are binary systems. Just to be honest our own Sun is a very weird star because it has no twin. If split this one, split also the others, but note again: Capella has six components and that alone is a very hard task. The number of astronomy articles may reach 50,000 or more once we split all star system acrticles. It's your choice if you want also to do a big job of splitting star systems, especially to close and visible stars. The decision is yours, my friends. Whatever it is, I will help. But I am telling you: once you split this you will start a large task. SkyFlubbler (talk) 02:18, 24 December 2014 (UTC)
  • Oppose – With a split, a summary of the discovery and system information would still need to remain, and so this action would not significantly reduce the article size. Besides, the article isn't overly lengthy, so the primary benefit of a split would be to expand upon the details of Sirius B. But that seems unlikely at present. The content on Sirius B is already well padded with general details on white dwarf stars. Praemonitus (talk) 17:34, 28 December 2014 (UTC)

Discussion

additional points separate from the survey on the split

If this is split, we will need to deregister the FA-status, as it will be a massive change to the article. (failure of the stability criterion, large changes in the content of the article) It should fall back to C-class or Start-class and start reassessment all over again (and the split off article should also not just copy "FA" over on its banners, but rated as Stub or Start class). -- 67.70.35.44 (talk) 11:42, 18 December 2014 (UTC)

Agreed, although I'd say B-class would be fine. StringTheory11 (t • c) 19:32, 27 December 2014 (UTC)
Presumably, if there is consensus for Tetra quark's proposal, it means carving up into three - a Sirius (star system) article, a Sirius A article and Sirius B article - and be hard to maintain as a threesome with much copying of information between three to keep them aligned - Tetra quark, where/how do you propose splitting. Is the system a disambiguation page? For instance, how would you propose carving up the System section - also, is all the cultural and visibility about the system or the brighter star? Cas Liber (talk · contribs) 21:15, 27 December 2014 (UTC)
My idea is not to have a page for the system. Let the Sirius article as it is (this article will actually be referring to Sirius A, which is a famous star for centuries) and create a new article for Sirius B, which is another star. We all know that we mean Sirius A when talking about Sirius. Tetra quark (talk) 01:28, 28 December 2014 (UTC)
I would disagree with your last statement. When we talk about "Sirius", we are talking about the system, not Sirius A. When we want to talk about Sirius A, we say "Sirius A", and when we want to talk about Sirius B, we say "Sirius B". StringTheory11 (t • c) 01:59, 28 December 2014 (UTC)
I still don't quite understand your point. We've known Sirius since prehistory, and now that we recently discovered Sirius B, now the word Sirius refers to the system? It doesn't matter if they are gravitationally interacting, they are two stars. It is almost like calling the Solar System "Sun". Tetra quark (talk) 12:53, 28 December 2014 (UTC)
now that we recently discovered Sirius B, now the word Sirius refers to the system? Yes. How we talk about things changes with the information we receive (hopefully, your thoughts, too, have been altered by the information in this discussion). Also, Sirius B was discovered in 1915.   ~ Tom.Reding (talk ⋅contribs ⋅dgaf)  13:49, 28 December 2014 (UTC)
Tetra quark, why would we then excise material on Sirius B from this article then? The two stars are intimately linked. Just because wr have a Geography of Ireland article doesn't mean we excise all material on geography from the Ireland article. Cas Liber (talk · contribs) 05:35, 28 December 2014 (UTC)

A comment on article prose size - the article currently has 28kb of prose, well under the size for considering splitting. Cas Liber (talk · contribs) 21:44, 27 December 2014 (UTC)

NB:The term is Wikipedia:Content forking, which is what we're trying to avoid. The chance of this is greatly increased with multiple articles. Cas Liber (talk · contribs) 21:47, 27 December 2014 (UTC)

The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Requested edit

The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Resolved after semiprotection expired

Please add a split template to the article subjectpage, since we are already discussing a split on the article above. -- 67.70.35.44 (talk) 11:33, 18 December 2014 (UTC)

Not done: According to the page's protection level and your user rights, you should be able to edit the page yourself. If you seem to be unable to, please reopen the request with further details. Neither that page, nor it's talk page have any kinds of protection on them and since they've been created already, you should be able to edit them. — {{U|Technical 13}} (e • t • c) 16:58, 18 December 2014 (UTC)
I already tried to edit the subjectpage Sirius to add the split template, it says "View Source" and This page is currently semi-protected so that only established registered users can edit it. when I click on View Source in case there was a caching problem ; the page also has a grey lock, indicating semiprotection (not red, indicating full protection, nor green, indicating move protection) I do see the protection log only indicating move protection, but I figure it must be cascaded protection or something. -- 67.70.35.44 (talk) 22:23, 18 December 2014 (UTC)
The page is indeed protected until tomorrow. Graeme Bartlett (talk) 11:10, 20 December 2014 (UTC)
Not done: The page's protection level and/or your user rights have changed since this request was placed. You should now be able to edit the page yourself. If you still seem to be unable to, please reopen the request with further details. Sam Sing! 17:17, 21 December 2014 (UTC)
The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Recent revision of magnitude?

On this so-called new revision of Hipparcos data, I've found the magnitude of Sirius to be -1.0876, which is quite a bit less than -1.46. What does that mean and should the article be updated?--Grondilu (talk) 13:07, 9 July 2015 (UTC)

Yeah, weird that. SIMBAD still has it as -1.46. Will see what else is out there discussing this...Cas Liber (talk · contribs) 19:08, 9 July 2015 (UTC)

- The HIPPARCOS magnitude is in a special bandpass unique to that instrument, it is not the V band. DEB 14 June 2016— Preceding unsigned comment added by 184.191.191.52 (talk) 14:15, 14 June 2016 (UTC)

The original Hipparcos catalogue includes a Johnson V magnitude (calculated, not measured) and gives it as −1.44 for Sirius. More generally, Simbad gives (usually, but not always!) a reference for the values they report such as magnitudes and radial velocities. You can then refer to that reference for comparison with any other catalogues you might be looking at. Simbad picks its values according to various criteria, and updates them from time to time. In this case, −1.46 is from the Bright Star Catalogue and from the Catalogue of Stellar Photometry in Johnson's 11-color system. Other papers have published slightly different values. The UBV Photoelectric Catalog (1987) lists values ranging from −1.40 to −1.47 and it would be a mistake to pick out any of them as "wrong". −1.46 is a widely accepted value, not least because it is the one in both Simbad (currently) and Wikipedia, but don't fall into the trap of thinking it is the "correct" or "only possible" value. Lithopsian (talk) 15:15, 14 June 2016 (UTC)

- There is another issue with the system and component apparent magnitudes listed in the top page's sidebar. The system V mag is given as -1.46, component A's V mag as -1.47 (citing a different reference), and component B's V mag as 8.44. But, those three values cannot all be correct. The system (sum of components A+B) must be brighter than component A alone. The problem lies in the uncertainties of stellar magnitudes, even (and maybe especially) for such a bright star, so reputable references can differ by 0.01 mags or more. Component B is 9100 times fainter in V band than component A, so to a precision of 0,01 mag it does not add to the system's apparent brightness. I suggest changing the component A apparent V magnitude to -1.46 and citing the same reference, #3, as given for the system's total brightness. DEB 14 June 2016.

They can all be "correct". There is an implicit margin of error with these measurements, not usually quoted explicitly, and reported V magnitudes from different sources will often vary by several hundredths of a magnitude. Your suggestion to calculate our own value for the magnitude of the primary component is not acceptable. Wikipedia should only report verifiable data, not things that we think we know. In this case, explicit measurements and reports of the magnitude of Sirius A are thin on the ground, not least for the reason you mention: that there is no point measuring something that can only be exactly the same as the combined magnitude. Feel free to find a reliable reference for the magnitude of Sirus A and B separately (preferably both from the same source), and cite it in the article. Make sure they are V magnitudes, but don't just cherry-pick. For example, the Tycho Double Star Catalogue (supplement) reports −1.09 for Sirius A, but nothing for Sirius B, and that is the value used in Simbad. Simbad is probably wrong to use this value as a V-band magnitude, because it is actually a Hipparcos-band magnitude as indicated by a flag in the Tycho catalogue. Lithopsian (talk) 15:15, 14 June 2016 (UTC)
SIMBAD also claims Radial Velocity is -5.5 km/s instead of -7.6 km/s ( BTW is this value supposed to be the full redshift, or can I expect the gravitational redshift to have been subtracted? For Sirius A I figure that would amount to ~ 800 m/s for light crawling up from gravitational well of the star. Hilmer B (talk) 21:38, 4 August 2015 (UTC)
Radial velocities are measured. They are not adjusted for intrinsic effects. Gravitational redshifts are present and should be at levels which can be measurable. Actual studies have failed to find a convincing contribution from gravitational redhsift, which should for example be noticeable as a statistical difference between main sequence (high gravity) and giant (low gravity) stars. Lithopsian (talk) 15:15, 14 June 2016 (UTC)
C'mon - you can't measure radial velocities like the Highway Patrol, not at these distances. You can measure red/blue-shift and then you may refer to it as "velocity" if you're not strict about what you're saying. So I think my question is still valid: Does Sirius A recede from us with 5.5 km/s or with 4.7 km/s? Hilmer B (talk) 21:15, 7 October 2016 (UTC)

First Section

"Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to increase, but it will continue to be the brightest star in the Earth's sky for the next 210,000 years."

Should the second sentence not read "After that time its distance will begin to decrease..." It doesn't seem to make sense with current wording. Texasjldavis (talk) 01:56, 9 February 2016 (UTC)

No, it starts to get further at 60,000 years but will still remain the brightest star. Cas Liber (talk · contribs) 02:25, 9 February 2016 (UTC)

The lead says this - that it will get closer then recede - but the more detailed section on distance fails to state HOW close it will get. Serious omission, I think. — Preceding unsigned comment added by 184.147.124.196 (talk) 18:00, 4 March 2016 (UTC)

Then fix it. It won't get much closer in comparison to its present difference. Doug Weller talk 18:33, 4 March 2016 (UTC)

Every edit I've ever made to wikipedia has been reverted back by some turf-defending dickhead, so why would I bother? (This article appears word-for-word all over the net, so one suspects it's plagiarized). In any case, according to https://en.wikipedia.org/wiki/Historical_brightest_stars , the minimum distance will be 7.8 ly, for those interested. Someone else can fix it. — Preceding unsigned comment added by 184.147.124.196 (talk) 18:41, 4 March 2016 (UTC)

That material should be in the body somewhere rather than the lead. I put most of this article together around 8 years ago, so am not surprised it's ended up all over the place. Damn...more reorganising needed.....Cas Liber (talk · contribs) 20:07, 4 March 2016 (UTC)
I agree. And it appears word for word elsewhere as it's being copied to other websites. Happens to a lot of our articles. Doug Weller talk 21:38, 4 March 2016 (UTC)

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Moved here from my talk page for discussion

Sirius

Original query from Worldandhistory:
Hi, sorry to pollute your TP with rather low importance matter, you may remove this section later, but I did not get your this undid as it is crucial, according to me, to mention that Sirius is also visible in day times in Polar Regions. For example, in some regions of Alaska, Sirius can be seen in daytime as well, same goes with some northwest extremities of Russia. When there is a full description required, a text may seem confusing but you can always correct the words and grammar rather than just removing the whole information. I can always say I was wrong but please re-conciser. :) Best - Worldandhistory (talk) 15:49, 28 September 2016 (UTC) Lithopsian (talk) 13:38, 29 September 2016 (UTC)

My thinking is that if it isn't the night sky, then the sun is brighter. Other editors apparently agree. Any other interpretation of day and night, polar or otherwise, is liable to confusion and would need more explanation than is appropriate in the opening sentence of the article. Lithopsian (talk) 11:22, 30 September 2016 (UTC)
Ok Lithopsian thank you for commenting. But can we elaborate this in the sub section of the article's page? Like in Visibility, though it is mentioned there that "Sirius can even be observed in daylight with the naked eye under the right conditions." If you or anyone else reading this opinion agrees, I would like to add the name of those regions. Don't you agree it's rather important to mention it's like a completely different definition for those readers who lives in those extremities regions, not just few but many people live there, uses Wiki and most of them are average readers. Just an opinion. Have a nice day! :) - Worldandhistory (talk) 01:27, 1 October 2016 (UTC)

ENGVAR

I was just having a tidy here when I noticed it is in a mixture of the two main spelling variants. I took a look through history and at this time it was in UK-Eng ("neighbour") and the various instances like "color" and "kilometer" have crept in since. Unless I am mistaken and there was a conscious decision to change it, I think per WP:RETAIN it should go back. It certainly cannot continue to have both variants. Thoughts? --John (talk) 23:42, 31 January 2017 (UTC)

On reflection , I just changed it back. --John (talk) 09:34, 1 February 2017 (UTC)

Eh, it could continue with both variants but this edit established the usage of the page as American English, so it's fine to stay consistent with that. Fixed. — LlywelynII 09:24, 9 February 2017 (UTC)
It couldn't, and that isn't what WP:RETAIN says. --John (talk) 19:11, 9 February 2017 (UTC)
  • I have returned the article to the dialect it was first written in as RETAIN mandates. Just as a point of information MoS compliance is an FA criterion. John (talk) 14:01, 14 February 2017 (UTC)

References

As a reminder, kindly don't use these on talk pages. — LlywelynII 15:10, 8 February 2017 (UTC)

Clarification and reference needed

This isn't referenced, and doesn't make sense.

The parallax of Sirius was measured by Thomas Henderson using his observations made in 1832–1833 and Maclear's observations made in 1836–1837, and was published in 1839. The value of the parallax was 0.23 arcseconds, and error of the parallax was estimated not to exceed a quarter of a second.

I almost just took it out. Does anyone have any suggestions? --John (talk) 21:24, 1 February 2017 (UTC)
I'll have a read of the sources later tonight when I have more than a few minutes to digest the reference. It's been years since I've looked at this article...Cas Liber (talk · contribs) 07:27, 2 February 2017 (UTC)
Thanks for anything you can do. 0.23 ± 0.25 isn't a very edifying data point for parallax since it includes zero. --John (talk) 08:25, 2 February 2017 (UTC)
It is edifying to the extent that it means Sirius is very likely at least 2 parsecs away. At the time, that was useful information. I'll add a reference direct to Henderson's publication. Henderson's letter makes it clear that detecting any parallax at all was worthwhile in itself. Lithopsian (talk) 14:58, 2 February 2017 (UTC)
I suppose so. It still looks silly as written, as the range includes zero. --John (talk) 22:19, 9 February 2017 (UTC)

I am not sure if I should create a new section for a small issue. I will put it here and I apologize if I should have created a new section. Does "8.60 ± 0.04 ly" mean it is 8.6 light years away? If so then I think that is an example of something that non-specialists would want to know but might not find/understand. The article about Alpha Centauri makes it clear that it/they (A and B) are 4.37 light years away. Sam Tomato (talk) 06:48, 11 March 2017 (UTC)

Merge

Near-unanimous consensus to proceed per the following steps-

The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Merge from Sothis to Sirius and/or Sopdet. There are weasel words in its article but Sothis is (and is universally regarded by RS as) the star Sirius, as already mentioned and sourced in the article Sirius. It is also ridiculous that the § Cultural significance section of the article Sirius currently has a paragraph on Theosophy, two subsections on minor African ethicities, and a Harry Potter shoutout but no discussion of its central importance to ancient Egyptian culture.

If it is felt important to maintain an entirely separate article on the ancient Egyptian cultural aspects of Sirius, it should occur at the star's ancient Egyptian name (typically reconstructed as Sopdet) and not at the romanization of the hellenization of that name. The current treatment there of the star as an Egyptian goddess should simply form a subsection of such an article, since she is simply a personification of the star within their culture. In that case, the § Cultural significance section of Sirius should still have an overview of the material being forked out and links to it. — LlywelynII 15:10, 8 February 2017 (UTC)

I just saw that there is an extended description of the goddess Sopdet in the § Observational history section. I footnoted it, but it probably should be dropped down to the § Cultural significance section when Egypt is added there. — LlywelynII 08:48, 9 February 2017 (UTC)

Yeah I think I agree with this. I'd be happy with either destination Cas Liber (talk · contribs) 09:17, 9 February 2017 (UTC)
Yes, a merge of some sort. Sothis as it stands is an article about Sirius under a different name and focusing on only a narrow aspect. Sirus already has a section on cultural significance where it would fit. Sopdet is about something that isn't a star and I think it should remain separate. Sopdet is already linked in the Sirius article (Sophis isn't) so it would take some care to keep the text consistent. Lithopsian (talk) 14:26, 9 February 2017 (UTC)


OK by me, but give some more time to see if other comments show up. It would seem to me suitable to put this as another bit in the Etymology and cultural significance section (with trimming of the Sothic Mythos bit,) and also to merge the See Also tags. Markbassett (talk) 23:51, 10 February 2017 (UTC)
Good point. Sourcing / removal of unsourced content could precede merging. Sothis cannot be left as is though, as it amounts to a wp:content fork, requiring deletion. Batternut (talk) 20:59, 26 February 2017 (UTC)
The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Fate of Sothis

Sorry. I didn't think this was unclear but the closing admin above didn't know what to do with Sothis after it's gutted.

Sothis should redirect to Sirius. The PRIMARYTOPIC of Sothis in English scholarship is historical discussion of the star itself, not its Egyptian or Hellenized deity. There can be a {{main}} hatnote in the § Name or § Cultural significance section that points anyone looking for the goddess Sothis to the Sopdet article. — LlywelynII 14:36, 10 March 2017 (UTC)

Fate of the "Sothic mythos" section

Some merge notes: the Sothic mythos stuff breaks crudely into (a) Iachen, (b) the destructive goddess, (c) dog attributes and the "Wolf Star" name. Having attempted/considered merging this section:

(a) The story of Iachen is unrelated to Sopdet and only peripherally related to Sirius. If deemed sufficiently notable of itself it could get its own article.
(b) Neither Sothis nor Sopdet are mentioned by the Kerenyi or Chamberlain sources.
(c) The Sirius article already mentions the "Wolf Star" name. The migration of the canis myth theory appears unsupported.

Thus I failed to find anything to merge. Batternut (talk) 11:20, 20 December 2017 (UTC)

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Adding a section on how our sun looks from this shstem

The article on Alpha Centauri has a fascinating section on what the sun would look like from one of its exoplanets.

Being a mere 8 light years away, I think it appropiate too add a similar section. NelsonWins (talk) 03:51, 4 July 2017 (UTC) NelsonWins (talk) 03:51, 4 July 2017 (UTC)

Morning Star as Other Designation

I noticed that nowhere in the article itself does it mention that Sirius has also been referred to as the Morning Star, similar to Venus. One of the bibliography titles shows the name, but nothing in the article. Also, when looking at https://en.wikipedia.org/wiki/Morning_Star it mentions it as an alternate name for Sirius.

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Southern

The Polynesians are said to be in the "Southern hemisphere". Most Polynesians are in the Southern hemisphere but Hawaii is north of the Equator. — Preceding unsigned comment added by 31.54.201.140 (talk) 06:45, 17 April 2018 (UTC)

Sirius A and B and other nomenclature difficulties

Sirius was, of course, the most commonly used traditional name for the point of light that also bears the Bayer designation Alpha Canis Majoris. When it was discovered to be a binary, the two components got the designations Alpha CMa A and B, often referred to as Sirius A and B. The article has obviously been written on that basis. However, in 2016 the International Astronomical Union set up a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. Thus the IAU now regards the name Sirius as applying only to the primary or 'A' component of Alpha CMa. As such, the term 'Sirius A' is both formally incorrect and misleading (Sirius doesn't have components). As for Sirius B, the WGSN stated that such informal names often attributed to other components in a physical multiple are treated as unofficial, albeit described as "useful nicknames".

Given the IAU's position as the internationally recognized authority for assigning designations and names to celestial bodies, its stance on this matter has to be reflected in the article (along with the traditional historical position), which therefore needs redrafting. I'm happy to do this myself, but as it's a significant change, I thought I'd raise it here first to garner any comments which I can reflect in the redrafting. One question is whether it would be better to change the article title to Alpha Canis Majoris (on balance, I'd say no, as 'Sirius' is far more commonly used). Cuddlyopedia (talk) 09:52, 30 July 2018 (UTC)

I wonder what it said about Capella then....but seriously, I see no problem with Sirius and Sirius B, which are by far the two most commonly used names. Cas Liber (talk · contribs) 10:36, 30 July 2018 (UTC)
The WGSN approved the name Capella for the brightest component (Alpha Aurigae Aa) so similar considerations apply. Quite a few of these star articles need amending, but I thought I'd start with Sirius as it's a simple system! :) Cuddlyopedia (talk) 09:31, 31 July 2018 (UTC)
The IAU is a widely-recognised body and its rulings have corresponding weight, but it isn't god and its working group doesn't change 100 years (I have refs going back to the 1920's but don't know who first used the term), and ongoing, widespread usage of the terms Sirius A and especially Sirius B. It doesn't even prohibit use of the term Sirius B, which could almost be called a proper name in itself, even if it isn't keen on these informal nicknames. We should describe what the IAU has said for completeness and accuracy, but I don't see the need for widespread renaming at this point. We certainly can't expunge the name Sirius B from existence. When even a modest number of people stop calling it Sirius B then we can consider whether to go further. It may be best now, and probably was previously anyway, to reduce usage of the term Sirius A except when it is necessary to explicitly distinguish from the companion. Lithopsian (talk) 12:30, 30 July 2018 (UTC)
As the change was made in 2016, it's not surprising most refs don't yet reflect it (how many refs are there that say Pluto is a planet? :) ). And I'm not proposing to expunge historical usage, but simply to reflect the change. Sirius B is regarded by the WGSN as an unofficial, albeit useful, nickname, so I see no problem in continuing to use it. Sirius A is another matter and apart from describing its historical usage, I suggest not using it. Sirius and Sirius B can always be distinguished if necessary using the Bayer designations or by use of the terms primary and secondary etc. Cuddlyopedia (talk) 09:31, 31 July 2018 (UTC)
The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.
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