Sources/First infrared source in Crux

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This infrared image from NASA's Spitzer Space Telescope shows the nebula nicknamed "the Dragonfish". Credit: NASA/JPL-Caltech/Univ. of Toronto.{{free media}}

The first infrared source in Crux is unknown.

The field of infrared astronomy is the result of observations and theories about infrared, or infrared-ray sources detected in the sky above.

The first astronomical infrared source discovered may have been the Sun.

But, infrared rays from the Sun are intermingled with other colors so that the Sun may appear yellow-white rather than infrared.

The early use of sounding rockets and balloons to carry infrared, optical, or visual detectors high enough may have detected infrared-rays from the Sun as early as the 1940s.

This is a lesson in map reading, coordinate matching, and searching. It is also a project in the history of infrared astronomy looking for the first astronomical infrared source discovered in the constellation of Crux.

Nearly all the background you need to participate and learn by doing you've probably already been introduced to at a secondary level and perhaps even a primary education level.

Some of the material and information is at the college or university level, and as you progress in finding infrared sources, you'll run into concepts and experimental tests that are an actual search.

First step[edit | edit source]

The first step is to succeed in finding an infrared source in Crux.

Next, you'll need to determine the time stamp of its discovery and compare it with any that have already been discovered.

Over the history of infrared astronomy a number of sources have been found, many as point sources in the night sky. These points are located on the celestial sphere using coordinate systems. Familiarity with these coordinate systems is not a prerequisite. Here the challenge is geometrical, astrophysical, and historical. The coordinates are usually supplied by the infrared source observers.

Astronomical sources[edit | edit source]

Def. a natural source usually of radiation in the sky especially at night is called an astronomical source.

A source of astronomical information on older detections of infrared sources is included in the Science section of the lecture/article infrared astronomy.

Traveling infrared sources[edit | edit source]

Many infrared sources do not remain in a constellation for lengthy periods. Some of these are the Sun and sources apparently in orbit around the Sun. The Sun travels through the 13 constellations along the ecliptic (the plane of the Earth's orbit around the Sun): the 12 of the Zodiac and the constellation Ophiuchus. These are described in source astronomy.

Backgrounds[edit | edit source]

To introduce yourself to some aspects of the challenge may I suggest reading the highlighted links mentioned above, and if you're curious, those listed under the section "See also" below.

Infrared-rays are a form of radiation that is currently part of the electromagnetic radiation intersecting the Earth. More information about radiation is in radiation astronomy.

Constellations[edit | edit source]

This is an image of the International Astronomical Union (IAU) sky map of the constellation Crux. Credit: IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg).{{free media}}

The Wikipedia article about the constellation Crux contains a high school level description. The figure at right shows the sky map of Crux. Around the edges of the map are coordinates related to longitude and latitude, but with the Earth rotating on its axis every 24 hours the celestial coordinates must remain fixed relative to the background light sources in the sky.

Also, in the Wikipedia article is a list of stars in Crux.

Searching catalogs[edit | edit source]

In the lecture/article infrared astronomy in its science section is a list of older catalogs of infrared sources. Using the constellation description in the previous section and the range of coordinates for the constellation in source astronomy, scan through the coordinates for these infrared sources to see if any may be within Crux.

If you find any that are, skip down to the section Infrared sources in Crux and make an entry. Be sure to check the coordinate era, most B1950 coordinates have changed slightly to the new J2000 set. Try the catalog designation at either SIMBAD website.

Testing a source[edit | edit source]

There are many web sites that may have an infrared source listed for the constellation Crux. Some that you may wish to try are in the External links section near the bottom of this lesson.

Wikipedia sources[edit | edit source]

A. Constellation article

Under "Notable features" in the Wikipedia article on the constellation Crux is the list of stars in Crux. Click on this link. In the table of this Wikipedia article is α Cru. To the right are coordinates:

Right ascension (RA): 12h 26m 35.94s and Declination (Dec): -63° 05' 56.6". Find these coordinates on the Crux map at the right.

To evaluate the star as an infrared-ray source, skip ahead to section "Infrared sources".

B. Wikipedia search

Another way to look for infrared sources in the constellation is to perform a search on Wikipedia. Try "Crux infrared" without the quotes. This yields about 26 returns which include an outline of astronomy and the Dragonfish nebula imaged in infrared at the top of this resource.

To evaluate each of these as an infrared source (or perhaps containing an infrared source, try your browser's "Find" feature and enter infrared or infrared-ray), skip ahead to section "Infrared sources".

SIMBAD sources[edit | edit source]

Another way to find possible infrared sources in Crux is to use search queries on SIMBAD.

Click on either SIMBAD link under "External links" below, then click on "Criteria query", or "by criteria".

In the tan box, type in "region(12 26 35.94 -63 05 56.6,10m)", without the quotes. This tells the SIMBAD computer you are interested in a circular region of the celestial sphere centered on the coordinates for alpha Crucis, with a radius of 10 arcminutes (m), or try 10d for 10 degrees.

Notice on the page over at the right from the tan colored box: "Return". The default is "object count". Click on "submit query". In a few moments a result something like "Number of objects: 32" should appear. Click "Back" to see the tan box again.

Adding "& otype='IR' to the region request reduces the returned number to 13.

The SIMBAD criteria search allows you to specify spectral types for possible stars. The criteria "sptype" (the exact spectral type): returns only the objects having the requested spectral type (i.e. sptype = 'k0' does not return 'K0III',...). And, "sptypes" should be used to retrive all objects having a spectral type containing the one specified; i.e., sptypes = 'K0' will return all objects having 'K0' as a spectral type, but also 'K0III' or 'K0IIIp', ...).

By comparing the (nm,temperature) pairs for the infrared range temperatures in the stellar classification in yellow astronomy suggests that the infrared range may be found from K8 through Y stars.

Add "sptypes='K9'" for example, to the entry so that it reads: "region(12 26 35.94 -63 05 56.6,10d) & sptypes='K9'", without the outside quotes. Click on "submit query" again. If the result is "0" number of objects, or "No object found", increase the number of arcminutes, or use "10d" which stands for "ten degrees".

When you find at least one object, change "Return" to "display" by clicking on the circle to its left, then "submit query".

SAO/NASA Astrophysics Data System[edit | edit source]

In the naming of sources per constellation, the genitive is in common use. For Crux, the genitive is Crucis.

Click on the SAO/NASA Astrophysics Data System link below in the "External links". Try "Crucis infrared" without the quotes, or "alpha crucis" with quotes, followed by infrared.

Click on a link below # Bibcode Authors. If the Abstract describes the detection of infrared-rays from a source in the constellation Crux, go to the next section under "SAO/NASA Astrophysics Data System".

If it does not try another bibcode link.

Infrared sources[edit | edit source]

There are several ways to evaluate an infrared source for the constellation Crux.

Wikipedia sources[edit | edit source]

Click on the link to the Wikipedia article. After you've enjoyed reading about the source, use the 'find' command of your browser to see if this Wikipedia page mentions anything about infrared, or "infrared-rays". Does the article mention whether or not the source is an infrared source?

What is the current time stamp for the Wikipedia article on the source? [Hint]: look for something like "This page was last modified on 25 December 2011 at 20:12." very near the bottom of the page. For now this is an adequate time stamp.

From reading the Wikipedia article on the source, if you believe the text demonstrates that the source is not an infrared source in Crux edit the "Non-infrared sources in Crux" section near the bottom of the page with an entry similar to "# Alpha Crucis 25 December 2011 at 20:12 Wikipedia article "Alpha Crucis", without the quotes, and finish the entry with four "~"s without the quotes after the period. The date included with your designation or username is a time stamp for the entry. The last portion of the entry is the source of your information.

On the other hand, if there are one or more sentences in the article that you believe demonstrates that the source is an infrared source in Crux edit the section below "Infrared sources in Crux" with a similar entry.

Go to the section entitled, "Challenging an entry".

Hint: the Wikipedia article on Alpha Crucis mentions, "Only two components are visually distinguishable, α1 and α2, separated by 4 arcseconds. α1 is magnitude 1.40 and α2 is magnitude 2.09, both hot class B (almost class O) stars, with surface temperatures of about 28,000 and 26,000 K respectively." From the lecture/article on infrared astronomy, the infrared radiation band the wavelength temperature pairs are approximately (750 nm, 4000 K) and (350000 nm, 8.6 K).

Is the primary star of alpha Crucis an infrared star?

Wikimedia commons[edit | edit source]

Another possible website for infrared sources is Wikimedia Commons, url=https://commons.wikimedia.org/wiki/Main_Page. Try entering "infrared Crux".

This returns six images of several infrared sources in Crux. These images often have sources with them indicated when the infrared image was obtained.

If there are one or more sentences in the article that you believe demonstrates that the source is an infrared source in Crux edit the section below "Infrared sources in Crux" with a similar entry mentioning the source from commons.

SIMBAD sources[edit | edit source]

To check any source (even one from Wikipedia) on SIMBAD, click of the "External link" to the "SIMBAD Astronomical Database".

At the lower right side of the SIMBAD Astronomical Database page is a "Basic search" box. There are several ways to try your target:

  1. source name: without the quotes or
  2. source coordinates: without the quotes, for example, "12 26 35.94 -63 05 56.6".

If you are looking at a SIMBAD generated table which lists possible targets, click on one.

On its SIMBAD page read down the left side until you see "Spectral type:". To the right of this is a designation. Look for a K-type star. Is there one?

If a K-star is present, skip down to the section, "SIMBAD time stamp". Even if a either is not present, noting that SIMBAD does not consider the source to be an infrared source is important, so skip down to the "SIMBAD time stamp" section.

If you have already found an infrared source (or a table of them) using SIMBAD, click on the blue link identifier for the first.

SIMBAD time stamp[edit | edit source]

Peruse the SIMBAD page for a time stamp or date of last revision. [Hint: it may look something like "2012.01.09CET20:10:02" and be in the upper right.]

If the entry at SIMBAD convinces you that the source is not an infrared source, edit the "Non-infrared sources in Crux" section near the bottom of this page and type in an entry similar to "# Source Name 2012.01.09CET20:10:02 SIMBAD article "SIMBAD source name".", without the first set of quotes, followed by four ~s.

If your SIMBAD analysis convinces you that you have found an infrared source in Crux (did you check the coordinates vs. the map of Crux?), make an entry something like the ones in the section "Infrared sources in Crux".

SAO/NASA Astrophysics Data System sources[edit | edit source]

If the abstract states that an infrared source in Crux is detected or studied, consider entering it in the section "Infrared sources in Crux" below.

Abstract time stamp[edit | edit source]

On the abstract page is a Publication Date:. This may serve as a time stamp for establishing that the source is detected as an infrared source on or before the date of publication. The time stamp followed by four ~s for your verification as determiner in the section "Infrared sources in Crux" completes your entry.

Challenging an entry[edit | edit source]

Any entry in either the section "Infrared sources in Crux" or "Non-infrared sources in Crux" can be challenged. The time stamp can be challenged to see if there is an earlier one. The source can be challenged by an earlier source.

Wikipedia challenges[edit | edit source]

Is Wikipedia a 'primary source', or does the Wikipedia article cite a source?

Even though Wikipedia has an article on the source, is it a good place to stop in testing whether the source has been detected as an astronomical infrared source?

If the Wikipedia article cites a primary source, skip down to the section on "Primary sources".

SIMBAD challenges[edit | edit source]

Is SIMBAD a 'primary source'?

SIMBAD is an astronomical database provided by the Centre de Données astronomiques de Strasbourg. It is an authoritative source, but they do occasionally make a mistake.

If you find an infrared source within the constellation on SIMBAD, the next step is to find the earliest time stamp of discovery.

SAO/NASA Astrophysics Data System challenge[edit | edit source]

Is the SAO/NASA Astrophysics Data System abstract entry a primary source?

The SAO/NASA Astrophysics Data System is an astronomical database provided by the High Energy Astrophysics Division at the Harvard-Smithsonian Center for Astrophysics of Harvard University. The abstract has been copied from the actual article in a scientific journal or other publication. Mistakes can be made and the article may record within its text exact dates when the observation or detection of infrared-rays actually occurred. Such a record may provide an earlier time stamp.

Primary sources[edit | edit source]

Primary sources may be searched for possible additional information perhaps not yet evaluated by SIMBAD or not presented in a Wikipedia article about a source.

Wikipedia test sources[edit | edit source]

For a Wikipedia article that cites a primary source, scroll down to the reference and open the reference. Read through the article looking for where the source mentioned in the Wikipedia article occurs. Some primary source authors may use source designations that are not mentioned in the Wikipedia article. To look for other designations, click on the link to SIMBAD in the "External links" on this page, enter the source name from the Wikipedia article, and see if other names are mentioned in the article.

When none of the names are mentioned, click on the link for "Google Advanced Search" in the list of "External links", enter the source name or designation(s) such as "Gliese 866", with "infrared-ray" to see if the source has a reference indicating it is an infrared source. And, look for the earliest one. Compose an entry using the primary source.

SIMBAD test sources[edit | edit source]

Further down the SIMBAD page is a list of "Identifiers". Click on the blue bold portion.

On the page that appears should be a primary source listed after Ref:. Click on the blue link with the oldest year. This yields an earlier time stamp and entry citation like the current one in the section "Infrared sources in Crux". If you find another source or an earlier time stamp, compose a similar entry and edit the section. Additional information to add into the reference can be found by clicking on "ADS services" from the SIMBAD page.

SAO/NASA Astrophysics Data System sources test[edit | edit source]

Click on either the "Electronic Refereed Journal Article (HTML)" or "Full Refereed Journal Article (PDF/Postscript)", if available.

Depending on the article display, if the abstract is repeated and the article is listed as FREE, click on either the PDF or HTML version.

While scanning or reading the article look for "Observations" (or use the Find function of your browser) and the possible inclusion of dates for these. If more than one infrared source in Crux are detected, which one(s) would you list in the section "Infrared sources in Crux" below?

An example of an article reference is provided in that section.

Changing an entry[edit | edit source]

From your analysis of the source so far, is it an infrared source?

If you have found an earlier time stamp for the source than the one listed in the section below "Non-infrared sources in Crux" and the answer to the above question is "no", you can edit the section with your result. Or, you can leave the entries as is and try another star.

If you have found an earlier time stamp for the source than the one listed in the section below "Infrared sources in Crux", edit the section with your result. Or, if you found another infrared source with a comparable or earlier time stamp, edit the section with your result.

Infrared sources in Crux[edit | edit source]

  1. HR 4731 SIMBAD: "C.D.S. - SIMBAD4 rel 1.218 - 2014.01.22CET03:17:15", "Object query : * alf02 Cru", SIMBAD lists the star's spectral type as "B1V", the otype is IR (2MASS). The infrared citation is 2003yCat.2246....0C. --Marshallsumter (discusscontribs) 02:30, 22 January 2014 (UTC)

Non-infrared sources in Crux[edit | edit source]

  1. Alpha Crucis, Wikipedia entry dated 13 January 2014 at 19:05 as the last update. "Acrux is a multiple star system located 321 light years from the earth.[1][2][7] Only two components are visually distinguishable, α1 and α2, separated by 4 arcseconds. α1 is magnitude 1.40 and α2 is magnitude 2.09, both hot class B (almost class O) stars, with surface temperatures of about 28,000 and 26,000 K respectively." A search of the entry using "infrared" turns up nothing. -- Marshallsumter (discusscontribs) 02:26, 22 January 2014 (UTC)

Oldest record[edit | edit source]

SIMBAD annotations[edit | edit source]

For any particular source, the SIMBAD record may indicate that it is not an infrared source yet above you may have found at least two refereed journal articles to indicate that it is. Use the second SIMBAD External links to directly display the SIMBAD database in France.

Enter the name source you have found into the search box. Scroll down to the Annotations :. Look for the link "add an annotation to this object". With browser open to the literature citations available, click on this link. You may need to register as a user. It's free. Post your annotation containing the literature references.

Hypotheses[edit | edit source]

  1. The first infrared source in Crux was probably observed around 200 b2k.

See also[edit | edit source]

External links[edit | edit source]

{{Radiation astronomy resources}}