70 Aquarii

{{short description|Star in the constellation Aquarius}}

{{Starbox begin}}

{{Starbox image

| image = 250px

| caption = The visual band light curve of 70 Aquarii, adapted from Weiss (1977)

}}

{{Starbox observe

| epoch=J2000

| ra={{RA|22|48|30.21043}}

| dec={{DEC|–10|33|19.7143}}

| appmag_v=6.19

| constell=Aquarius

}}

{{Starbox character

| type=main sequencec

| class=F0 V

| b-v=+0.28

| u-b=

| variable=δ Sct

}}

{{Starbox astrometry

| radial_v=–5.8

| prop_mo_ra=+31.535

| prop_mo_dec=+7.915

| parallax=7.6654

| p_error=0.0704

| parallax_footnote=

| absmag_v=+0.88

}}

{{Starbox detail

| mass=

| radius={{Val|4.17|0.17|0.23}}

| luminosity={{Val|44.8|0.5}}

| temperature={{Val|7314|187|144|fmt=commas}}

| metal_fe={{Val|0.02|0.15}}

| gravity=3.48

| rotational_velocity=110

| age_myr=

}}

{{Starbox catalog

| names={{odlist | F=70 Aqr | BD=−11°5923 | FK5=3825 | HD=215874 | HIP=112615 | HR=8676 | SAO=165308 }}

}}

{{Starbox reference

| Simbad=70+Aqr

}}

{{Starbox end}}

70 Aquarii is a variable star located 425 light years away from the Sun in the equatorial constellation of Aquarius. It has the variable star designation FM Aquarii; 70 Aquarii is the Flamsteed designation. It is near the lower limit of visibility to the naked eye, appearing as a dim, yellow-white hued star with a baseline apparent visual magnitude of 6.19. This star is moving closer to the Earth with a heliocentric radial velocity of –5.8 km/s.

Werner Wolfgang Weiss discovered that 70 Aquarii was a variable star in 1977. It was given its variable star designation in 1981.

This is an F-type main-sequence star with a stellar classification of F0 V. Located in the lower part of the instability strip, it is a Delta Scuti-type variable that ranges in brightness from magnitude 6.16 down to 6.19 with a period of {{Convert|0.087|days|minutes|abbr=off|order=flip}}. The star has a high rate of spin, showing a projected rotational velocity of 110 km/s. It has four times the Sun's radius and is radiating 45 times the luminosity of the Sun from its photosphere at an effective temperature of around 7,314 K.

References

{{reflist|refs=

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| arxiv=1604.07403 | s2cid=119241004

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{{cite simbad | title=70 Aqr | access-date=2019-05-19 }}

}}