HR3724
HR3724 is a variable and multiple star in the constellation of Hydra.
HR3724 visual magnitude is 6.53. Because of its reltive faintness, HR3724 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR3724:
HR3724 is below the horizon from Greenwich, United Kingdom .
Altitude: -37.5°
Azimuth: 51.9°
Direction: North-East
Celestial coordinates and finder chart of HR3724
HR3724 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR3724 are provided in the following table:
The simplified sky map below shows the position of HR3724 in the sky:

Visibility of HR3724 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR3724 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR3724
The image below is a photograph of HR3724 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of HR3724 is -0.027 arcsec per year in Right Ascension and -0.021 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR3724 from the Sun and relative movement
HR3724 is distant 452.78 light years from the Sun and it is moving far from the Sun at the speed of 23 kilometers per second.
Spectral properties of HR3724
HR3724 belongs to spectral class A5 HR3724 is also a SrCrEu chemically peculiar star.
The red dot in the diagram below shows where HR3724 is situated in the Hertzsprung–Russell diagram.

HR3724 star system properties
HR3724 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR3724 double sysyem: