Basics of Using a Telescope - Locating Stars (RA)

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Discussion Overview

The discussion revolves around the concept of Right Ascension (RA) in astronomy, particularly in relation to locating stars using a telescope. Participants explore the definition of RA, its measurement, and the implications of Earth's movement on the apparent positions of celestial objects. The conversation includes both theoretical understanding and practical implications for stargazing.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that RA is measured eastwards from the point where the Sun crosses the celestial equator at the vernal equinox, questioning if a star behind the Sun at that moment would have an RA of zero.
  • There is a discussion about the variability of RA for planets, with some participants suggesting that this is due to both the Earth's movement around the Sun and the planets' own movements.
  • One participant questions whether a planet's RA changes by 4 minutes each day, leading to clarification that this is not solely the case due to the planets' own motions.
  • Participants note that while stars appear fixed, their RA can change slowly due to the precession of the Earth's axis and the proper motion of nearby stars.
  • There is a query regarding the units of RA, specifically whether one hour of RA corresponds to one arc hour, with clarification that one hour of RA equals 15 degrees, but minutes and seconds differ from arc units.

Areas of Agreement / Disagreement

Participants generally agree on the basic definition of RA and its measurement, but there are varying interpretations regarding the implications of planetary motion and the changes in RA over time. The discussion remains unresolved on some technical details, particularly regarding the relationship between RA and angular measure units.

Contextual Notes

Participants express uncertainty about the changing nature of RA for celestial objects and the implications of Earth's movement. There are limitations in the discussion regarding the precise definitions and conversions between time and angular units.

Jimmy87
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Hello pf,

I have been trying to grasp the concept of RA. I have read through a few books and I know that it is measured eastwards from the point on the celestial sphere where the Sun crosses the celestial equator at the vernal equinox. I just want to check I understand this correctly. Does it mean when the Sun cross the celestial equator, whatever star happens to be behind the Sun at that point would serve as a RA of zero?

My other query is whenever you look up right ascensions on the internet or a phone app they are always constantly changing (or at least for planets)? Again I tried to research this with little luck but is it because nearby objects e.g. planets appear to not stay at the same point in the sky day to day because the Earth moves around the Sun (which is why a solar day is 4 minutes longer). So a planet would change its right ascension by 4 minutes each day? But a star is so much further away it will be fixed?

Any help is much appreciated.
 
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Jimmy87 said:
Hello pf,

I have been trying to grasp the concept of RA. I have read through a few books and I know that it is measured eastwards from the point on the celestial sphere where the Sun crosses the celestial equator at the vernal equinox. I just want to check I understand this correctly. Does it mean when the Sun cross the celestial equator, whatever star happens to be behind the Sun at that point would serve as a RA of zero?

Yes.

My other query is whenever you look up right ascensions on the internet or a phone app they are always constantly changing (or at least for planets)? Again I tried to research this with little luck but is it because nearby objects e.g. planets appear to not stay at the same point in the sky day to day because the Earth moves around the Sun (which is why a solar day is 4 minutes longer).

Yes, but also because the planets themselves are moving around the sun.

So a planet would change its right ascension by 4 minutes each day?

No, because the planet itself is also moving.

But a star is so much further away it will be fixed?

Yes, approximately. But the RA of stars also change slowly for two reasons. First, the precession of the Earth's axis causes the coordinate system to rotate slowly, causing RA's to change on the order of 1 degree per century. Second, nearby stars do move slowly because they are not infinitely far away. This is called proper motion, and is typically on the order of seconds of arc per year.
 
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phyzguy said:
Yes.
Yes, but also because the planets themselves are moving around the sun.
No, because the planet itself is also moving.
Yes, approximately. But the RA of stars also change slowly for two reasons. First, the precession of the Earth's axis causes the coordinate system to rotate slowly, causing RA's to change on the order of 1 degree per century. Second, nearby stars do move slowly because they are not infinitely far away. This is called proper motion, and is typically on the order of seconds of arc per year.
Thank you for your help it is much appreciated. When RA is quoted it is given in units of time because 360 degrees is treated as 24 hours. Are these units of time the same as arc units (e.g. is one hour of RA one arc hour) or are these units for RA different to units of arc?
 
Jimmy87 said:
Thank you for your help it is much appreciated. When RA is quoted it is given in units of time because 360 degrees is treated as 24 hours. Are these units of time the same as arc units (e.g. is one hour of RA one arc hour) or are these units for RA different to units of arc?
It can be very confusing. One hour of RA is 15 degrees. This is not too bad. But one minute of RA is different from one minute of arc, and one second of RA is different from one second of arc. Attached is a brief description that I wrote for a class I taught a couple of years ago. Table 1 gives the correspondence between units of RA and angular measure.
 

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