There exist people that doubt or doesn't believe or simply don't know that Earth orbits Sun. This web-site is done for those people.
RZ CAS is famous variable star, eclipsing binary or fotometric double star, in constellation of Cassiopeia. It is double star so that they orbit each other at about 1.195252 days period. RZ CAS rounds 305.6 cycles in one Earth's year. Eclipsings are easily observable visually by typical 10x50 binoculars. Minima are deep and fast which makes it possible to get reasonable minute-accurate minima even without special expensive equipments.
All you need are : eyes, watch, binoculars, star chart with magnitudes, ephemerides(predicted approx. minima times),notebook, pencil, CAREFUL PATIENCE and calculator.
I have been observing double star RZ Cas for over four years since 3 May 1997. Personally observed 39 single geocentric minima show such regular variation that man can get only one conclusion: Earth is moving.
RZ Cas is never behind the Sun but high up at about 50 degrees angle compared to Earth's orbit level. So light travel difference time between Earth and Sun is never greater than cos(50)*8.3 min = approx 5.3 minutes.
Situation can be visualized this way:

Fig.1. On 28 May every year the Earth is on the farthest point from RZ CAS
point of view. Light pulses get to the Sun 5.3 minutes earlier than to the Earth.

Fig.2. On 28 November every year the Earth is on the closest point from RZ CAS
point of view. Light pulses get to the Sun 5.3 minutes later than to the Earth. It means Observed values should be 5.3 less (O-C=-5.3) than expected from
Earth citizen's point of view.
Respectively on 25 February and 30 August every year the Sun and the Earth are at the same distance from RZ Cas's point of view and light time difference is 0.
In fact if heliocentric hypothesis is right then minima times should be heaving back and forth approx. at 5.3 amplitude according to sine wave when someone observes RZ Cas minima on the Earth. On the other hand if geocentric hypothese is right and heliocentric hypothesis is wrong then minima times should not be waving on such yearly period at all. Only "small" random variation.
Here we can see my personally observed 40 minima O-C values of RZCAS.
Observed-Calculated (O-C) means observed versus (linearly) predicted.
I have used 1.195252d as predicted period (Source was Kari Kaila:
Tahtitaivaan opas, URSA (Finnish)). And On 3 May 1997 heliocentric
minimum HelioJudianDate 50571.422971 was as starting zeropoint O-C for my
graphs.
If minima happens for ex. 4.6 minutes later than predicted
then it is marked O-C=+4.6 min.
| Date [ddmmyy] | Time[hh.mm.des]+-acc[min] FINTIME (UT+2h) | GeoJulianDate | Geocentric O-C [min] | Light-time delay [min] | Heliocentric O-C [min] | Cycles from first minimum |
|---|---|---|---|---|---|---|
| 03.05.1997 | 00.14.0+-6m | 50571.426389 | +4.92 | -4.92 | 0.00 | 0 |
| 09.08.1997 | 00.25.0+-2m | 50669.4340 | +0.64 | -1.84 | -1.28 | 82 |
| 14.08.1997 | 23.49.6+-3m | 50675.4094 | -0.65 | -1.32 | -1.97 | 87 |
| 26.08.1997 | 22.41.5+-4m | 50687.3622 | -0.38 | -0.25 | -0.63 | 97 |
| 19.02.1998 | 20.14.4+-4m | 50864.2600 | +0.41 | +0.50 | +0.91 | 245 |
| 27.02.1998 | 00.23.4+-4m | 50871.4329 | +2.44 | -0.17 | +2.27 | 251 |
| 05.04.1998 | 01.42.1+-2m | 50908.4876 | +5.09 | -3.34 | +1.75 | 282 |
| 22.09.1998 | 23.41.6+-6m | 51079.4039 | -1.70 | +2.12 | +0.42 | 425 |
| 04.10.1998 | 22.33.0+-4m | 51091.3563 | -1.93 | +3.07 | +1.14 | 435 |
| 09.11.1998 | 19.07.6+-4m | 51127.2136 | -2.22 | +4.99 | +2.77 | 465 |
| 22.12.1998 | 19.52.3+-1m | 51170.2446 | +0.62 | +4.78 | +5.40 | 501 |
| 24.12.1998 | 00.28.1+-2m | 51171.4362 | +4.72 | +4.73 | -0.01 | 502 |
| 09.01.1999 | 18.08.6+-4m | 51188.1726 | -0.52 | +3.86 | +3.34 | 516 |
| 10.01.1999 | 22.46.7+-2m | 51189.3658 | -3.58 | +3.78 | +0.20 | 517 |
| 28.01.1999 | 21.06.6+-3m | 51207.2963 | -1.13 | +2.46 | +1.33 | 532 |
| 11.02.1999 | 00.40.3+-2m | 51220.4447 | -0.22 | +1.32 | +1.10 | 543 |
| 17.02.1999 | 00.06.1+-2m | 51226.4209 | -0.24 | +0.78 | +0.54 | 548 |
| 06.03.1999 | 22.26.6+-4m | 51244.3518 | +2.82 | -0.87 | +1.95 | 563 |
| 12.03.1999 | 21.53.2+-2m | 51250.3286 | +3.61 | -1.42 | +2.19 | 568 |
| 14.03.1999 | 02.32.0+-2m | 51251.5222 | +1.24 | -1.52 | -0.28 | 569 |
| 26.03.1999 | 01.25.2+-2m | 51263.4758 | +2.81 | -2.54 | +0.27 | 579 |
| 12.04.1999 | 23.45.2+-2m | 51281.4064 | +5.37 | -3.86 | +1.51 | 594 |
| 24.04.1999 | 22.40.2+-4m | 51293.36125 | +8.74 | -4.55 | +4.19 | 604 |
| 26.08.1999 | 01.13.4+-3m | 51416.4676 | +2.17 | -0.38 | +1.79 | 707 |
| 07.09.1999 | 00.01.7+-5m | 51428.4178 | -1.17 | +0.71 | -0.46 | 717 |
| 12.09.1999 | 23.29.5+-3m | 51434.39548 | +0.82 | +1.24 | +2.06 | 722 |
| 06.10.1999 | 21.13.8+-4m | 51458.30125 | +1.87 | +3.19 | +5.06 | 742 |
| 18.10.1999 | 20.01.6+-4m | 51470.2511 | -1.97 | +3.99 | +2.02 | 752 |
| 02.12.1999 | 01.24.7+-2m | 51514.4755 | -1.89 | +5.25 | +3.36 | 789 |
| 08.12.1999 | 00.48.6+-3m | 51520.4504 | -3.80 | +5.19 | +1.39 | 794 |
| 30.12.1999 | 17.48.2+-2m | 51543.1585 | -6.30 | +4.44 | -1.86 | 813 |
| 18.01.2000 | 20.53.1+-2m | 51562.28687 | -0.01 | +3.26 | +3.25 | 829 |
| 24.01.2000 | 20.08.8+-7m* | 51568.25611 | -10.12 | +2.80 | -7.32 | 834* |
| 14.02.2000 | 03.59.5+-2m | 51588.58299 | +0.81 | +1.06 | +1.87 | 851 |
| 24.02.2000 | 22.09.3+-5m | 51599.33979 | +0.15 | +0.07 | +0.22 | 860 |
| 26.02.2000 | 02.52.0+-3m | 51600.53646 | +2.18 | -0.04 | +2.14 | 861 |
| 03.03.2000 | 02.17.7+-2m | 51606.51229 | +1.57 | -0.59 | +0.98 | 866 |
| 21.03.2000 | 00.35.2+-3m | 51624.44111 | +1.62 | -2.19 | -0.57 | 881 |
| 27.03.2000 | 00.03.0+-4m | 51630.41875 | +3.61 | -2.68 | +0.93 | 886 |
| 01.04.2000 | 23.29.8+-4m | 51636.39569 | +4.60 | -3.15 | +1.45 | 891 |
I omitted one point(*) from graphs. It was very cloudy sky and accuracy very poor. Normally man should not observe variable stars on such poor weather but I tried to look if it affects accuracy. It did.
These are not just my personal data anymore. First 10 minima points are reported to AAVSO, the rest are reported in Swiss Astronomical Society and appeared (and to appear) in BBSAG Bulletins. Closer look to my observations and links to my scientific observations of variable stars can be found at astrov.html.
Here we can see observed minima in cycles vs O-C graphs. Blue spikes mark approximate typical (95%-)accuracy (+-3 minutes) of my minima observations.

Fig.3.Geocentric plot. Observed points (yellow dots) are plotted as they are seen
from Earth. The blue sine wave is theoretical heliocentric light-time model
to explain varying dots. Blue spikes show +-3 minute accuracy borders.
Remark how well dots fit to heliocentric explanation curve. Earth is really moving and minima pulses are really waving according to light time effect as it should.

Fig.4.Heliocentric plot. Points are plotted from Sun's (calculated)
point of view. Light time effect is mathematically decreased from points
and we can see here that dots fit reasonable well to mildly increasing
line(slope). And most of them fit to the slope within 3 minutes accuracy.
Slightly increasing slope means that RZ Cas has in recent years shown
little longer period (1.195270d) than was predicted (1.195252d) in literature.
Some refinements: Actually you can see that arc of parabole would fit better than straight line. RZ CAS is making some very long period O-C. Fortunately it stayed quite constant for 4 years. Perhaps later I analyse for accurate, fit parabola and get good estimate of speed of light of distant star from my 39 measurements !
Doupter of heliocentricity should explain me how come it is possible:
This article was written by Mr. Kari A.Tikkanen with Emacs-editor on 9
October 2000 in Oulu.
(c) K.A.T. 2000.